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http://hdl.handle.net/2248/4643
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DC Field | Value | Language |
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dc.contributor.author | Sivarani, T | - |
dc.contributor.author | Parthasarathy, M | - |
dc.contributor.author | García, L. P | - |
dc.contributor.author | Manchado, A | - |
dc.date.accessioned | 2009-07-15T16:06:20Z | - |
dc.date.available | 2009-07-15T16:06:20Z | - |
dc.date.issued | 2001-08 | - |
dc.identifier.citation | Szczerba, R. and Garny, S. K., eds., Post-AGB objects as a phase of stellar evolution, Astrophysics and Space Science Library, Vol. 265, Proceedings of the Torun Workshop held July 5 - 7, 2000, pp. 305 – 308 | en |
dc.identifier.isbn | 0-7923-7145-3 | - |
dc.identifier.uri | http://hdl.handle.net/2248/4643 | - |
dc.description | Restricted Access | - |
dc.description.abstract | IRAS 10215-5916 was classified as a post-AGB star and also as a massive red supergiant. It was also found to be a spectroscopic binary. In our high resolution spectra we found molecular features from a cool star of Teff = 3750K. We also see the spectral signature of a relatively hotter star of Teff = 7250K. We found that both the components of the binary system are metal poor. From the theoretical spectrum synthesis we obtained [C/H] = -0.2 +/- 0.4, [O/H] = -1.0 +/- 0.4 and [Fe/H] = -2.0 +/- 0.5 for the hot component of the binary system. The enhanced carbon abundance and metal poor characteristics show that the hot component of the binary system could be a post-AGB star. | en |
dc.language.iso | en | en |
dc.publisher | Kluwer Academic Publishers | en |
dc.relation.ispartofseries | Astrophysics and Space Science Library; Vol. 265 | - |
dc.relation.uri | http://adsabs.harvard.edu/abs/2001ASSL..265..305S | en |
dc.subject | Spectroscopy of Post-AGB | en |
dc.subject | IRAS 10215-5916 | en |
dc.title | Spectroscopy of post-AGB candidate IRAS 10215-5916 | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
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File | Description | Size | Format | |
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Spectroscopy of post-AGB candidate IRAS 10215-5916 Restricted Access | Restricted Access | 105.79 kB | Adobe PDF | View/Open Request a copy |
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