Modelling of the spectra and atmospheres of evolved stars
| dc.creator | Pavlenko, Yakiv V. | |
| dc.date | 2006-06-11 | |
| dc.date.accessioned | 2026-07-07T07:12:11Z | |
| dc.date.available | 2026-07-07T07:12:11Z | |
| dc.description | The method and results of the computation of the model atmospheres and spectral energy distributions of chemically peculiar stars, are discussed. The models are computed with a special consideration of the particular problems encountered when computing model atmospheres for M and C-giants, and of hydrogen deficient stars. We present some computed model atmospheres for Sakurai's object, giants of globular clusters, and C-giants. | |
| dc.description | To be published in Memorie della Societa' Astronomica Italiana, as a contributed talk for the VIII Torino Workshop on Nucleosynthesis in AGB Stars "Constraints on AGB Nucleosynthesis from Observations" Granada, 5-10 February 2006 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0606252 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0606252 | |
| dc.identifier | Mem.Soc.Ast.It. 75 (2004) 282 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/111995 | |
| dc.subject | Astrophysics | |
| dc.title | Modelling of the spectra and atmospheres of evolved stars | |
| dc.type | text |