Spectroscopy of post-AGB star IRAS 01005+7910
Infrared source IRAS 01005+7910 is identified with an 11-mag peculiar star which has been previously found to be a post asymptotic giant branch star of early spectral type. There is significant spectral variability detected earlier. Over 30 spectra were obtained with high resolution (15000 − 60000)...
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| Veröffentlicht in: | Advances in Astronomy and Space Physics |
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| Datum: | 2011 |
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| Format: | Artikel |
| Sprache: | Englisch |
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Advances in astronomy and space physics
2011
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/118940 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Spectroscopy of post-AGB star IRAS 01005+7910 / D.S. Nasonov // Advances in astronomy and space physics. — 2011. — Т. 1., вип. 1-2. — С. 5-8. — Бібліогр.: 12 назв. — англ. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| _version_ | 1862740231447379968 |
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| author | Nasonov, D.S. |
| author_facet | Nasonov, D.S. |
| citation_txt | Spectroscopy of post-AGB star IRAS 01005+7910 / D.S. Nasonov // Advances in astronomy and space physics. — 2011. — Т. 1., вип. 1-2. — С. 5-8. — Бібліогр.: 12 назв. — англ. |
| collection | DSpace DC |
| container_title | Advances in Astronomy and Space Physics |
| description | Infrared source IRAS 01005+7910 is identified with an 11-mag peculiar star which has been previously found to be a post asymptotic giant branch star of early spectral type. There is significant spectral variability detected earlier. Over 30 spectra were obtained with high resolution (15000 − 60000) in spectral range 3500 − 7800 ˚A˚A. In this work the results of the spectral monitoring of this object are presented. The detailed analysis of radial velocities was carried out. Radial velocities derived from different absorption lines show variability within the same spectrum. Significant variability of radial velocities is demonstrated on the scale of one day. The variability of line profiles is present. The constant radial velocity −51 ± 1.4 km/s of forbidden lines was detected. Shell expansion velocity is estimated from widths of forbidden emission line profiles. The hydrogen and helium line profiles demonstrate the complicated and changing picture both of accretion and outflow in envelope.
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| first_indexed | 2025-12-07T20:13:56Z |
| format | Article |
| fulltext | |
| id | nasplib_isofts_kiev_ua-123456789-118940 |
| institution | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| isbn | 987-966-439-367-3 |
| language | English |
| last_indexed | 2025-12-07T20:13:56Z |
| publishDate | 2011 |
| publisher | Advances in astronomy and space physics |
| record_format | dspace |
| spelling | Nasonov, D.S. 2017-06-01T15:00:52Z 2017-06-01T15:00:52Z 2011 Spectroscopy of post-AGB star IRAS 01005+7910 / D.S. Nasonov // Advances in astronomy and space physics. — 2011. — Т. 1., вип. 1-2. — С. 5-8. — Бібліогр.: 12 назв. — англ. 987-966-439-367-3 https://nasplib.isofts.kiev.ua/handle/123456789/118940 Infrared source IRAS 01005+7910 is identified with an 11-mag peculiar star which has been previously found to be a post asymptotic giant branch star of early spectral type. There is significant spectral variability detected earlier. Over 30 spectra were obtained with high resolution (15000 − 60000) in spectral range 3500 − 7800 ˚A˚A. In this work the results of the spectral monitoring of this object are presented. The detailed analysis of radial velocities was carried out. Radial velocities derived from different absorption lines show variability within the same spectrum. Significant variability of radial velocities is demonstrated on the scale of one day. The variability of line profiles is present. The constant radial velocity −51 ± 1.4 km/s of forbidden lines was detected. Shell expansion velocity is estimated from widths of forbidden emission line profiles. The hydrogen and helium line profiles demonstrate the complicated and changing picture both of accretion and outflow in envelope. This work was supported in part by Russian Foundation for Basic Research (project 08-02-00072) en Advances in astronomy and space physics Advances in Astronomy and Space Physics Physics of Stars and Galaxies Spectroscopy of post-AGB star IRAS 01005+7910 Article published earlier |
| spellingShingle | Spectroscopy of post-AGB star IRAS 01005+7910 Nasonov, D.S. Physics of Stars and Galaxies |
| title | Spectroscopy of post-AGB star IRAS 01005+7910 |
| title_full | Spectroscopy of post-AGB star IRAS 01005+7910 |
| title_fullStr | Spectroscopy of post-AGB star IRAS 01005+7910 |
| title_full_unstemmed | Spectroscopy of post-AGB star IRAS 01005+7910 |
| title_short | Spectroscopy of post-AGB star IRAS 01005+7910 |
| title_sort | spectroscopy of post-agb star iras 01005+7910 |
| topic | Physics of Stars and Galaxies |
| topic_facet | Physics of Stars and Galaxies |
| url | https://nasplib.isofts.kiev.ua/handle/123456789/118940 |
| work_keys_str_mv | AT nasonovds spectroscopyofpostagbstariras010057910 |