Photometric study of the FUor star V 1735 Cyg (Elias 1-12)
Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present d...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Peneva, S. P. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2009 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© Springer Science+Business Media B.V. 2009 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 323(2009), 4 vom: 02. Sept., Seite 329-335 |
|---|---|
| Übergeordnetes Werk: |
volume:323 ; year:2009 ; number:4 ; day:02 ; month:09 ; pages:329-335 |
| Links: |
|---|
| DOI / URN: |
10.1007/s10509-009-0078-7 |
|---|
| Katalog-ID: |
OLC2066257028 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2066257028 | ||
| 003 | DE-627 | ||
| 005 | 20230502213608.0 | ||
| 007 | tu | ||
| 008 | 200820s2009 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/s10509-009-0078-7 |2 doi | |
| 035 | |a (DE-627)OLC2066257028 | ||
| 035 | |a (DE-He213)s10509-009-0078-7-p | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 520 |a 530 |a 620 |q VZ |
| 084 | |a 16,12 |2 ssgn | ||
| 100 | 1 | |a Peneva, S. P. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Photometric study of the FUor star V 1735 Cyg (Elias 1-12) |
| 264 | 1 | |c 2009 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
| 338 | |a Band |b nc |2 rdacarrier | ||
| 500 | |a © Springer Science+Business Media B.V. 2009 | ||
| 520 | |a Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. | ||
| 650 | 4 | |a Pre-main sequence stars | |
| 650 | 4 | |a T Tauri stars | |
| 650 | 4 | |a V 1735 Cyg | |
| 700 | 1 | |a Semkov, E. H. |4 aut | |
| 700 | 1 | |a Stavrev, K. Y. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astrophysics and space science |d Springer Netherlands, 1968 |g 323(2009), 4 vom: 02. Sept., Seite 329-335 |w (DE-627)129062723 |w (DE-600)629-4 |w (DE-576)014393522 |x 0004-640X |7 nnns |
| 773 | 1 | 8 | |g volume:323 |g year:2009 |g number:4 |g day:02 |g month:09 |g pages:329-335 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/s10509-009-0078-7 |z lizenzpflichtig |3 Volltext |
| 912 | |a GBV_USEFLAG_A | ||
| 912 | |a SYSFLAG_A | ||
| 912 | |a GBV_OLC | ||
| 912 | |a SSG-OLC-TEC | ||
| 912 | |a SSG-OLC-PHY | ||
| 912 | |a SSG-OLC-AST | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_40 | ||
| 912 | |a GBV_ILN_47 | ||
| 912 | |a GBV_ILN_70 | ||
| 912 | |a GBV_ILN_2279 | ||
| 912 | |a GBV_ILN_4012 | ||
| 951 | |a AR | ||
| 952 | |d 323 |j 2009 |e 4 |b 02 |c 09 |h 329-335 | ||
| author_variant |
s p p sp spp e h s eh ehs k y s ky kys |
|---|---|
| matchkey_str |
article:0004640X:2009----::htmtisuyfhfosav7 |
| hierarchy_sort_str |
2009 |
| publishDate |
2009 |
| allfields |
10.1007/s10509-009-0078-7 doi (DE-627)OLC2066257028 (DE-He213)s10509-009-0078-7-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Peneva, S. P. verfasserin aut Photometric study of the FUor star V 1735 Cyg (Elias 1-12) 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. Pre-main sequence stars T Tauri stars V 1735 Cyg Semkov, E. H. aut Stavrev, K. Y. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 323(2009), 4 vom: 02. Sept., Seite 329-335 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:323 year:2009 number:4 day:02 month:09 pages:329-335 https://doi.org/10.1007/s10509-009-0078-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 323 2009 4 02 09 329-335 |
| spelling |
10.1007/s10509-009-0078-7 doi (DE-627)OLC2066257028 (DE-He213)s10509-009-0078-7-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Peneva, S. P. verfasserin aut Photometric study of the FUor star V 1735 Cyg (Elias 1-12) 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. Pre-main sequence stars T Tauri stars V 1735 Cyg Semkov, E. H. aut Stavrev, K. Y. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 323(2009), 4 vom: 02. Sept., Seite 329-335 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:323 year:2009 number:4 day:02 month:09 pages:329-335 https://doi.org/10.1007/s10509-009-0078-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 323 2009 4 02 09 329-335 |
| allfields_unstemmed |
10.1007/s10509-009-0078-7 doi (DE-627)OLC2066257028 (DE-He213)s10509-009-0078-7-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Peneva, S. P. verfasserin aut Photometric study of the FUor star V 1735 Cyg (Elias 1-12) 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. Pre-main sequence stars T Tauri stars V 1735 Cyg Semkov, E. H. aut Stavrev, K. Y. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 323(2009), 4 vom: 02. Sept., Seite 329-335 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:323 year:2009 number:4 day:02 month:09 pages:329-335 https://doi.org/10.1007/s10509-009-0078-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 323 2009 4 02 09 329-335 |
| allfieldsGer |
10.1007/s10509-009-0078-7 doi (DE-627)OLC2066257028 (DE-He213)s10509-009-0078-7-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Peneva, S. P. verfasserin aut Photometric study of the FUor star V 1735 Cyg (Elias 1-12) 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. Pre-main sequence stars T Tauri stars V 1735 Cyg Semkov, E. H. aut Stavrev, K. Y. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 323(2009), 4 vom: 02. Sept., Seite 329-335 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:323 year:2009 number:4 day:02 month:09 pages:329-335 https://doi.org/10.1007/s10509-009-0078-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 323 2009 4 02 09 329-335 |
| allfieldsSound |
10.1007/s10509-009-0078-7 doi (DE-627)OLC2066257028 (DE-He213)s10509-009-0078-7-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Peneva, S. P. verfasserin aut Photometric study of the FUor star V 1735 Cyg (Elias 1-12) 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. Pre-main sequence stars T Tauri stars V 1735 Cyg Semkov, E. H. aut Stavrev, K. Y. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 323(2009), 4 vom: 02. Sept., Seite 329-335 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:323 year:2009 number:4 day:02 month:09 pages:329-335 https://doi.org/10.1007/s10509-009-0078-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 323 2009 4 02 09 329-335 |
| language |
English |
| source |
Enthalten in Astrophysics and space science 323(2009), 4 vom: 02. Sept., Seite 329-335 volume:323 year:2009 number:4 day:02 month:09 pages:329-335 |
| sourceStr |
Enthalten in Astrophysics and space science 323(2009), 4 vom: 02. Sept., Seite 329-335 volume:323 year:2009 number:4 day:02 month:09 pages:329-335 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Pre-main sequence stars T Tauri stars V 1735 Cyg |
| dewey-raw |
520 |
| isfreeaccess_bool |
false |
| container_title |
Astrophysics and space science |
| authorswithroles_txt_mv |
Peneva, S. P. @@aut@@ Semkov, E. H. @@aut@@ Stavrev, K. Y. @@aut@@ |
| publishDateDaySort_date |
2009-09-02T00:00:00Z |
| hierarchy_top_id |
129062723 |
| dewey-sort |
3520 |
| id |
OLC2066257028 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066257028</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213608.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2009 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-009-0078-7</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066257028</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10509-009-0078-7-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Peneva, S. P.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Photometric study of the FUor star V 1735 Cyg (Elias 1-12)</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2009</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science+Business Media B.V. 2009</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Pre-main sequence stars</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">T Tauri stars</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">V 1735 Cyg</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Semkov, E. H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stavrev, K. Y.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Springer Netherlands, 1968</subfield><subfield code="g">323(2009), 4 vom: 02. Sept., Seite 329-335</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:323</subfield><subfield code="g">year:2009</subfield><subfield code="g">number:4</subfield><subfield code="g">day:02</subfield><subfield code="g">month:09</subfield><subfield code="g">pages:329-335</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s10509-009-0078-7</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">323</subfield><subfield code="j">2009</subfield><subfield code="e">4</subfield><subfield code="b">02</subfield><subfield code="c">09</subfield><subfield code="h">329-335</subfield></datafield></record></collection>
|
| author |
Peneva, S. P. |
| spellingShingle |
Peneva, S. P. ddc 520 ssgn 16,12 misc Pre-main sequence stars misc T Tauri stars misc V 1735 Cyg Photometric study of the FUor star V 1735 Cyg (Elias 1-12) |
| authorStr |
Peneva, S. P. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)129062723 |
| format |
Article |
| dewey-ones |
520 - Astronomy & allied sciences 530 - Physics 620 - Engineering & allied operations |
| delete_txt_mv |
keep |
| author_role |
aut aut aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0004-640X |
| topic_title |
520 530 620 VZ 16,12 ssgn Photometric study of the FUor star V 1735 Cyg (Elias 1-12) Pre-main sequence stars T Tauri stars V 1735 Cyg |
| topic |
ddc 520 ssgn 16,12 misc Pre-main sequence stars misc T Tauri stars misc V 1735 Cyg |
| topic_unstemmed |
ddc 520 ssgn 16,12 misc Pre-main sequence stars misc T Tauri stars misc V 1735 Cyg |
| topic_browse |
ddc 520 ssgn 16,12 misc Pre-main sequence stars misc T Tauri stars misc V 1735 Cyg |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| hierarchy_parent_title |
Astrophysics and space science |
| hierarchy_parent_id |
129062723 |
| dewey-tens |
520 - Astronomy 530 - Physics 620 - Engineering |
| hierarchy_top_title |
Astrophysics and space science |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)129062723 (DE-600)629-4 (DE-576)014393522 |
| title |
Photometric study of the FUor star V 1735 Cyg (Elias 1-12) |
| ctrlnum |
(DE-627)OLC2066257028 (DE-He213)s10509-009-0078-7-p |
| title_full |
Photometric study of the FUor star V 1735 Cyg (Elias 1-12) |
| author_sort |
Peneva, S. P. |
| journal |
Astrophysics and space science |
| journalStr |
Astrophysics and space science |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science 600 - Technology |
| recordtype |
marc |
| publishDateSort |
2009 |
| contenttype_str_mv |
txt |
| container_start_page |
329 |
| author_browse |
Peneva, S. P. Semkov, E. H. Stavrev, K. Y. |
| container_volume |
323 |
| class |
520 530 620 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Peneva, S. P. |
| doi_str_mv |
10.1007/s10509-009-0078-7 |
| dewey-full |
520 530 620 |
| title_sort |
photometric study of the fuor star v 1735 cyg (elias 1-12) |
| title_auth |
Photometric study of the FUor star V 1735 Cyg (Elias 1-12) |
| abstract |
Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. © Springer Science+Business Media B.V. 2009 |
| abstractGer |
Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. © Springer Science+Business Media B.V. 2009 |
| abstract_unstemmed |
Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly. © Springer Science+Business Media B.V. 2009 |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 |
| container_issue |
4 |
| title_short |
Photometric study of the FUor star V 1735 Cyg (Elias 1-12) |
| url |
https://doi.org/10.1007/s10509-009-0078-7 |
| remote_bool |
false |
| author2 |
Semkov, E. H. Stavrev, K. Y. |
| author2Str |
Semkov, E. H. Stavrev, K. Y. |
| ppnlink |
129062723 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/s10509-009-0078-7 |
| up_date |
2024-07-04T04:05:20.637Z |
| _version_ |
1803619842811494400 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066257028</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213608.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2009 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-009-0078-7</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066257028</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10509-009-0078-7-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Peneva, S. P.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Photometric study of the FUor star V 1735 Cyg (Elias 1-12)</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2009</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science+Business Media B.V. 2009</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Results from optical photometric observations of the PMS star V 1735 Cyg are reported. The star is located in the IC 5146 dark cloud complex—a region of active star formation. On the basis of observed outburst and spectral properties, V 1735 Cyg was classified as a FUor object. We present data from BVRI CCD photometric observations of the star, collected from March 2003 to January 2009. Plates from the Rozhen Schmidt telescope archive were scanned for a brightness estimation of the star. A sequence of sixteen comparison stars in the field of V 1735 Cyg was calibrated in BVRI bands. The data from photographic observations made from 1986 to 1992 show a strong light variability (ΔV=1⋅m2). In contrast, the recent photometric data obtained from 2003 to 2009 show only small amplitude variations (ΔI=0⋅m3). The analysis of existing photometric data shows a very slow decrease in star brightness—1⋅m8 (R) for a 44 year period. The possibilities for future photometric investigations of V 1735 Cyg using the photographical plate archives is discussed briefly.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Pre-main sequence stars</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">T Tauri stars</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">V 1735 Cyg</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Semkov, E. H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stavrev, K. Y.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Springer Netherlands, 1968</subfield><subfield code="g">323(2009), 4 vom: 02. Sept., Seite 329-335</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:323</subfield><subfield code="g">year:2009</subfield><subfield code="g">number:4</subfield><subfield code="g">day:02</subfield><subfield code="g">month:09</subfield><subfield code="g">pages:329-335</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s10509-009-0078-7</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">323</subfield><subfield code="j">2009</subfield><subfield code="e">4</subfield><subfield code="b">02</subfield><subfield code="c">09</subfield><subfield code="h">329-335</subfield></datafield></record></collection>
|
| score |
7.399583 |