Stellar spectroscopy methods for study of supernova remnants
We present the method for study of the characteristics of the supernova remnants using their absorption properties. The background radiation sources are several stars with wide range of distances. Main task is accurate extraction of stellar spectra from observations. For Vela Jr. supernova remnant w...
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| Published in: | Advances in Astronomy and Space Physics |
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| Date: | 2011 |
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| Format: | Article |
| Language: | English |
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Advances in astronomy and space physics
2011
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| Online Access: | https://nasplib.isofts.kiev.ua/handle/123456789/118943 |
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| Cite this: | Stellar spectroscopy methods for study of supernova remnants / Yu.V. Pakhomov, N.N. Chugai, A.F. Iyudin // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 15-18. — Бібліогр.: 7 назв. — англ. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
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Pakhomov, Yu.V. Chugai, N.N. Iyudin, A.F. 2017-06-01T15:11:50Z 2017-06-01T15:11:50Z 2011 Stellar spectroscopy methods for study of supernova remnants / Yu.V. Pakhomov, N.N. Chugai, A.F. Iyudin // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 15-18. — Бібліогр.: 7 назв. — англ. 987-966-439-367-3 https://nasplib.isofts.kiev.ua/handle/123456789/118943 We present the method for study of the characteristics of the supernova remnants using their absorption properties. The background radiation sources are several stars with wide range of distances. Main task is accurate extraction of stellar spectra from observations. For Vela Jr. supernova remnant we found the absence of typical broad absorption in the spectral lines of Ca ii doublet. Using modeles of supernovae remnants and data on radiation in ⁴⁴Ti γ-ray line we estimated the age and the distance to Vela Jr. We showed that a hypernova may be a probable candidate for Vela Jr. protogenitor. en Advances in astronomy and space physics Advances in Astronomy and Space Physics Physics of Stars and Galaxies Stellar spectroscopy methods for study of supernova remnants Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Stellar spectroscopy methods for study of supernova remnants |
| spellingShingle |
Stellar spectroscopy methods for study of supernova remnants Pakhomov, Yu.V. Chugai, N.N. Iyudin, A.F. Physics of Stars and Galaxies |
| title_short |
Stellar spectroscopy methods for study of supernova remnants |
| title_full |
Stellar spectroscopy methods for study of supernova remnants |
| title_fullStr |
Stellar spectroscopy methods for study of supernova remnants |
| title_full_unstemmed |
Stellar spectroscopy methods for study of supernova remnants |
| title_sort |
stellar spectroscopy methods for study of supernova remnants |
| author |
Pakhomov, Yu.V. Chugai, N.N. Iyudin, A.F. |
| author_facet |
Pakhomov, Yu.V. Chugai, N.N. Iyudin, A.F. |
| topic |
Physics of Stars and Galaxies |
| topic_facet |
Physics of Stars and Galaxies |
| publishDate |
2011 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Advances in astronomy and space physics |
| format |
Article |
| description |
We present the method for study of the characteristics of the supernova remnants using their absorption properties. The background radiation sources are several stars with wide range of distances. Main task is accurate extraction of stellar spectra from observations. For Vela Jr. supernova remnant we found the absence of typical broad absorption in the spectral lines of Ca ii doublet. Using modeles of supernovae remnants and data on radiation in ⁴⁴Ti γ-ray line we estimated the age and the distance to Vela Jr. We showed that a hypernova may be a probable candidate for Vela Jr. protogenitor.
|
| isbn |
987-966-439-367-3 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/118943 |
| citation_txt |
Stellar spectroscopy methods for study of supernova remnants / Yu.V. Pakhomov, N.N. Chugai, A.F. Iyudin // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 15-18. — Бібліогр.: 7 назв. — англ. |
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AT pakhomovyuv stellarspectroscopymethodsforstudyofsupernovaremnants AT chugainn stellarspectroscopymethodsforstudyofsupernovaremnants AT iyudinaf stellarspectroscopymethodsforstudyofsupernovaremnants |
| first_indexed |
2025-12-02T00:21:26Z |
| last_indexed |
2025-12-02T00:21:26Z |
| _version_ |
1850861265623187456 |