Study of the late nitrogen-sequence Galactic Wolf–Rayet star WR156. Spectropolarimetry and modeling
• Galactic Wolf–Rayet star WR156 is studied spectropolarimetrically for the first time. • We measured the polarization and position angle and did not found any line effect. • The polarization detected by us is of interstellar origin. • We modelled the wind of WR156 and derived the parameters of its...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Maryeva, O.V. [verfasserIn] |
|---|
| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2013 |
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| Schlagwörter: |
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| Umfang: |
5 |
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| Übergeordnetes Werk: |
Enthalten in: Tracking of informative gamma frequency range in local field potentials of anesthetized rat olfactory bulb for odor discrimination - Shepelev, Igor ELSEVIER, 2021, an international journal in astronomy and astrophysics, [Amsterdam] |
|---|---|
| Übergeordnetes Werk: |
volume:25 ; year:2013 ; pages:27-31 ; extent:5 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.newast.2013.03.015 |
|---|
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ELV038522810 |
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| 520 | |a • Galactic Wolf–Rayet star WR156 is studied spectropolarimetrically for the first time. • We measured the polarization and position angle and did not found any line effect. • The polarization detected by us is of interstellar origin. • We modelled the wind of WR156 and derived the parameters of its atmosphere. • As a result, WR156 is the richest hydrogen Wolf–Rayet star of WN8 type in the Galaxy. | ||
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10.1016/j.newast.2013.03.015 doi GBVA2013002000015.pica (DE-627)ELV038522810 (ELSEVIER)S1384-1076(13)00041-9 DE-627 ger DE-627 rakwb eng 520 520 DE-600 610 VZ 44.09 bkl 44.32 bkl Maryeva, O.V. verfasserin aut Study of the late nitrogen-sequence Galactic Wolf–Rayet star WR156. Spectropolarimetry and modeling 2013 5 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier • Galactic Wolf–Rayet star WR156 is studied spectropolarimetrically for the first time. • We measured the polarization and position angle and did not found any line effect. • The polarization detected by us is of interstellar origin. • We modelled the wind of WR156 and derived the parameters of its atmosphere. • As a result, WR156 is the richest hydrogen Wolf–Rayet star of WN8 type in the Galaxy. WR156 stars Elsevier Wolf–Rayet Elsevier Stars Elsevier Individual Elsevier Polarimetric techniques Elsevier Afanasiev, V.L. oth Panchuk, V.E. oth Enthalten in Elsevier Science Shepelev, Igor ELSEVIER Tracking of informative gamma frequency range in local field potentials of anesthetized rat olfactory bulb for odor discrimination 2021 an international journal in astronomy and astrophysics [Amsterdam] (DE-627)ELV006757626 volume:25 year:2013 pages:27-31 extent:5 https://doi.org/10.1016/j.newast.2013.03.015 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.09 Medizintechnik VZ 44.32 Medizinische Mathematik medizinische Statistik VZ AR 25 2013 27-31 5 045F 520 |
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10.1016/j.newast.2013.03.015 doi GBVA2013002000015.pica (DE-627)ELV038522810 (ELSEVIER)S1384-1076(13)00041-9 DE-627 ger DE-627 rakwb eng 520 520 DE-600 610 VZ 44.09 bkl 44.32 bkl Maryeva, O.V. verfasserin aut Study of the late nitrogen-sequence Galactic Wolf–Rayet star WR156. Spectropolarimetry and modeling 2013 5 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier • Galactic Wolf–Rayet star WR156 is studied spectropolarimetrically for the first time. • We measured the polarization and position angle and did not found any line effect. • The polarization detected by us is of interstellar origin. • We modelled the wind of WR156 and derived the parameters of its atmosphere. • As a result, WR156 is the richest hydrogen Wolf–Rayet star of WN8 type in the Galaxy. WR156 stars Elsevier Wolf–Rayet Elsevier Stars Elsevier Individual Elsevier Polarimetric techniques Elsevier Afanasiev, V.L. oth Panchuk, V.E. oth Enthalten in Elsevier Science Shepelev, Igor ELSEVIER Tracking of informative gamma frequency range in local field potentials of anesthetized rat olfactory bulb for odor discrimination 2021 an international journal in astronomy and astrophysics [Amsterdam] (DE-627)ELV006757626 volume:25 year:2013 pages:27-31 extent:5 https://doi.org/10.1016/j.newast.2013.03.015 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.09 Medizintechnik VZ 44.32 Medizinische Mathematik medizinische Statistik VZ AR 25 2013 27-31 5 045F 520 |
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Study of the late nitrogen-sequence Galactic Wolf–Rayet star WR156. Spectropolarimetry and modeling |
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• Galactic Wolf–Rayet star WR156 is studied spectropolarimetrically for the first time. • We measured the polarization and position angle and did not found any line effect. • The polarization detected by us is of interstellar origin. • We modelled the wind of WR156 and derived the parameters of its atmosphere. • As a result, WR156 is the richest hydrogen Wolf–Rayet star of WN8 type in the Galaxy. |
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• Galactic Wolf–Rayet star WR156 is studied spectropolarimetrically for the first time. • We measured the polarization and position angle and did not found any line effect. • The polarization detected by us is of interstellar origin. • We modelled the wind of WR156 and derived the parameters of its atmosphere. • As a result, WR156 is the richest hydrogen Wolf–Rayet star of WN8 type in the Galaxy. |
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• Galactic Wolf–Rayet star WR156 is studied spectropolarimetrically for the first time. • We measured the polarization and position angle and did not found any line effect. • The polarization detected by us is of interstellar origin. • We modelled the wind of WR156 and derived the parameters of its atmosphere. • As a result, WR156 is the richest hydrogen Wolf–Rayet star of WN8 type in the Galaxy. |
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