ASTEC—the Aarhus STellar Evolution Code
Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been careful...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Christensen-Dalsgaard, Jørgen [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2007 |
|---|
| Schlagwörter: |
|---|
| Anmerkung: |
© Springer Science+Business Media B.V. 2007 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 316(2007), 1-4 vom: 25. Dez., Seite 13-24 |
|---|---|
| Übergeordnetes Werk: |
volume:316 ; year:2007 ; number:1-4 ; day:25 ; month:12 ; pages:13-24 |
| Links: |
|---|
| DOI / URN: |
10.1007/s10509-007-9675-5 |
|---|
| Katalog-ID: |
OLC2066254495 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | OLC2066254495 | ||
| 003 | DE-627 | ||
| 005 | 20230502213545.0 | ||
| 007 | tu | ||
| 008 | 200820s2007 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.1007/s10509-007-9675-5 |2 doi | |
| 035 | |a (DE-627)OLC2066254495 | ||
| 035 | |a (DE-He213)s10509-007-9675-5-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 Christensen-Dalsgaard, Jørgen |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a ASTEC—the Aarhus STellar Evolution Code |
| 264 | 1 | |c 2007 | |
| 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. 2007 | ||
| 520 | |a Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. | ||
| 650 | 4 | |a Stars | |
| 650 | 4 | |a Stellar structure | |
| 650 | 4 | |a Stellar evolution | |
| 773 | 0 | 8 | |i Enthalten in |t Astrophysics and space science |d Springer Netherlands, 1968 |g 316(2007), 1-4 vom: 25. Dez., Seite 13-24 |w (DE-627)129062723 |w (DE-600)629-4 |w (DE-576)014393522 |x 0004-640X |7 nnns |
| 773 | 1 | 8 | |g volume:316 |g year:2007 |g number:1-4 |g day:25 |g month:12 |g pages:13-24 |
| 856 | 4 | 1 | |u https://doi.org/10.1007/s10509-007-9675-5 |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_2286 | ||
| 912 | |a GBV_ILN_4012 | ||
| 951 | |a AR | ||
| 952 | |d 316 |j 2007 |e 1-4 |b 25 |c 12 |h 13-24 | ||
| author_variant |
j c d jcd |
|---|---|
| matchkey_str |
article:0004640X:2007----::seteahstlaeo |
| hierarchy_sort_str |
2007 |
| publishDate |
2007 |
| allfields |
10.1007/s10509-007-9675-5 doi (DE-627)OLC2066254495 (DE-He213)s10509-007-9675-5-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Christensen-Dalsgaard, Jørgen verfasserin aut ASTEC—the Aarhus STellar Evolution Code 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2007 Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. Stars Stellar structure Stellar evolution Enthalten in Astrophysics and space science Springer Netherlands, 1968 316(2007), 1-4 vom: 25. Dez., Seite 13-24 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:316 year:2007 number:1-4 day:25 month:12 pages:13-24 https://doi.org/10.1007/s10509-007-9675-5 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_2286 GBV_ILN_4012 AR 316 2007 1-4 25 12 13-24 |
| spelling |
10.1007/s10509-007-9675-5 doi (DE-627)OLC2066254495 (DE-He213)s10509-007-9675-5-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Christensen-Dalsgaard, Jørgen verfasserin aut ASTEC—the Aarhus STellar Evolution Code 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2007 Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. Stars Stellar structure Stellar evolution Enthalten in Astrophysics and space science Springer Netherlands, 1968 316(2007), 1-4 vom: 25. Dez., Seite 13-24 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:316 year:2007 number:1-4 day:25 month:12 pages:13-24 https://doi.org/10.1007/s10509-007-9675-5 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_2286 GBV_ILN_4012 AR 316 2007 1-4 25 12 13-24 |
| allfields_unstemmed |
10.1007/s10509-007-9675-5 doi (DE-627)OLC2066254495 (DE-He213)s10509-007-9675-5-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Christensen-Dalsgaard, Jørgen verfasserin aut ASTEC—the Aarhus STellar Evolution Code 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2007 Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. Stars Stellar structure Stellar evolution Enthalten in Astrophysics and space science Springer Netherlands, 1968 316(2007), 1-4 vom: 25. Dez., Seite 13-24 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:316 year:2007 number:1-4 day:25 month:12 pages:13-24 https://doi.org/10.1007/s10509-007-9675-5 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_2286 GBV_ILN_4012 AR 316 2007 1-4 25 12 13-24 |
| allfieldsGer |
10.1007/s10509-007-9675-5 doi (DE-627)OLC2066254495 (DE-He213)s10509-007-9675-5-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Christensen-Dalsgaard, Jørgen verfasserin aut ASTEC—the Aarhus STellar Evolution Code 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2007 Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. Stars Stellar structure Stellar evolution Enthalten in Astrophysics and space science Springer Netherlands, 1968 316(2007), 1-4 vom: 25. Dez., Seite 13-24 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:316 year:2007 number:1-4 day:25 month:12 pages:13-24 https://doi.org/10.1007/s10509-007-9675-5 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_2286 GBV_ILN_4012 AR 316 2007 1-4 25 12 13-24 |
| allfieldsSound |
10.1007/s10509-007-9675-5 doi (DE-627)OLC2066254495 (DE-He213)s10509-007-9675-5-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Christensen-Dalsgaard, Jørgen verfasserin aut ASTEC—the Aarhus STellar Evolution Code 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2007 Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. Stars Stellar structure Stellar evolution Enthalten in Astrophysics and space science Springer Netherlands, 1968 316(2007), 1-4 vom: 25. Dez., Seite 13-24 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:316 year:2007 number:1-4 day:25 month:12 pages:13-24 https://doi.org/10.1007/s10509-007-9675-5 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_2286 GBV_ILN_4012 AR 316 2007 1-4 25 12 13-24 |
| language |
English |
| source |
Enthalten in Astrophysics and space science 316(2007), 1-4 vom: 25. Dez., Seite 13-24 volume:316 year:2007 number:1-4 day:25 month:12 pages:13-24 |
| sourceStr |
Enthalten in Astrophysics and space science 316(2007), 1-4 vom: 25. Dez., Seite 13-24 volume:316 year:2007 number:1-4 day:25 month:12 pages:13-24 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| topic_facet |
Stars Stellar structure Stellar evolution |
| dewey-raw |
520 |
| isfreeaccess_bool |
false |
| container_title |
Astrophysics and space science |
| authorswithroles_txt_mv |
Christensen-Dalsgaard, Jørgen @@aut@@ |
| publishDateDaySort_date |
2007-12-25T00:00:00Z |
| hierarchy_top_id |
129062723 |
| dewey-sort |
3520 |
| id |
OLC2066254495 |
| 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">OLC2066254495</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213545.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2007 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-007-9675-5</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066254495</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10509-007-9675-5-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">Christensen-Dalsgaard, Jørgen</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">ASTEC—the Aarhus STellar Evolution Code</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2007</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. 2007</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stars</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar structure</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar evolution</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">316(2007), 1-4 vom: 25. Dez., Seite 13-24</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:316</subfield><subfield code="g">year:2007</subfield><subfield code="g">number:1-4</subfield><subfield code="g">day:25</subfield><subfield code="g">month:12</subfield><subfield code="g">pages:13-24</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s10509-007-9675-5</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_2286</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">316</subfield><subfield code="j">2007</subfield><subfield code="e">1-4</subfield><subfield code="b">25</subfield><subfield code="c">12</subfield><subfield code="h">13-24</subfield></datafield></record></collection>
|
| author |
Christensen-Dalsgaard, Jørgen |
| spellingShingle |
Christensen-Dalsgaard, Jørgen ddc 520 ssgn 16,12 misc Stars misc Stellar structure misc Stellar evolution ASTEC—the Aarhus STellar Evolution Code |
| authorStr |
Christensen-Dalsgaard, Jørgen |
| 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 |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0004-640X |
| topic_title |
520 530 620 VZ 16,12 ssgn ASTEC—the Aarhus STellar Evolution Code Stars Stellar structure Stellar evolution |
| topic |
ddc 520 ssgn 16,12 misc Stars misc Stellar structure misc Stellar evolution |
| topic_unstemmed |
ddc 520 ssgn 16,12 misc Stars misc Stellar structure misc Stellar evolution |
| topic_browse |
ddc 520 ssgn 16,12 misc Stars misc Stellar structure misc Stellar evolution |
| 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 |
ASTEC—the Aarhus STellar Evolution Code |
| ctrlnum |
(DE-627)OLC2066254495 (DE-He213)s10509-007-9675-5-p |
| title_full |
ASTEC—the Aarhus STellar Evolution Code |
| author_sort |
Christensen-Dalsgaard, Jørgen |
| 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 |
2007 |
| contenttype_str_mv |
txt |
| container_start_page |
13 |
| author_browse |
Christensen-Dalsgaard, Jørgen |
| container_volume |
316 |
| class |
520 530 620 VZ 16,12 ssgn |
| format_se |
Aufsätze |
| author-letter |
Christensen-Dalsgaard, Jørgen |
| doi_str_mv |
10.1007/s10509-007-9675-5 |
| dewey-full |
520 530 620 |
| title_sort |
astec—the aarhus stellar evolution code |
| title_auth |
ASTEC—the Aarhus STellar Evolution Code |
| abstract |
Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. © Springer Science+Business Media B.V. 2007 |
| abstractGer |
Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. © Springer Science+Business Media B.V. 2007 |
| abstract_unstemmed |
Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing. © Springer Science+Business Media B.V. 2007 |
| 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_2286 GBV_ILN_4012 |
| container_issue |
1-4 |
| title_short |
ASTEC—the Aarhus STellar Evolution Code |
| url |
https://doi.org/10.1007/s10509-007-9675-5 |
| remote_bool |
false |
| ppnlink |
129062723 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1007/s10509-007-9675-5 |
| up_date |
2024-07-04T04:05:00.250Z |
| _version_ |
1803619821422641152 |
| 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">OLC2066254495</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213545.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2007 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-007-9675-5</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066254495</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10509-007-9675-5-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">Christensen-Dalsgaard, Jørgen</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">ASTEC—the Aarhus STellar Evolution Code</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2007</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. 2007</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The Aarhus code is the result of a long development, starting in 1974, and still ongoing. A novel feature is the integration of the computation of adiabatic oscillations for specified models as part of the code. It offers substantial flexibility in terms of microphysics and has been carefully tested for the computation of solar models. However, considerable development is still required in the treatment of nuclear reactions, diffusion and convective mixing.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stars</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar structure</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar evolution</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">316(2007), 1-4 vom: 25. Dez., Seite 13-24</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:316</subfield><subfield code="g">year:2007</subfield><subfield code="g">number:1-4</subfield><subfield code="g">day:25</subfield><subfield code="g">month:12</subfield><subfield code="g">pages:13-24</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s10509-007-9675-5</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_2286</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">316</subfield><subfield code="j">2007</subfield><subfield code="e">1-4</subfield><subfield code="b">25</subfield><subfield code="c">12</subfield><subfield code="h">13-24</subfield></datafield></record></collection>
|
| score |
7.401063 |