Issue |
EAS Publications Series
Volume 71-72, 2015
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
|
|
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Page(s) | 155 - 158 | |
Section | Binaries | |
DOI | https://doi.org/10.1051/eas/1571034 | |
Published online | 01 December 2015 |
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 155-158
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 155-158
SMC3 As a Test To The Binary Evolution
1 Nicolaus Copernicus Astronomical Centre, Bartycka 18, 00716 Warsaw, Poland
2 Warsaw University Observatory, Al. Ujazdowskie 4, 00–478 Warszawa, Poland
SMC 3 is one of the most interesting symbiotic stars. This binary contains a bright K-type giant transferring mass to a massive white dwarf comanion, which makes it is a very promising SN Ia candidate. We discuss the evolutionary status of the system using results of population synthesis code.
© EAS, EDP Sciences, 2015