Evolution of a binary system consisting of a helium star and a white dwarf

Details Evolution of a binary system consisting of a helium star and a white dwarf Evolution of a binary system consisting of a helium star and a white dwarf

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.163..143e&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 163, no. 1, Jan. 1990, p. 143-152.

Astronomy and Astrophysics

Astrophysics

10

B Stars, Binary Stars, Roche Limit, Stellar Evolution, White Dwarf Stars, Cataclysmic Variables, Mass Transfer, Stellar Mass Accretion, Thermal Instability

Scientific paper

Results are presented from evolutionary calculations for a close binary system with a central helium burning He-star filling its Roche lobe and an accreting white (CO) dwarf. It is suggested that these systems may be presupernovae for certain SN I types. To examine this hypothesis, evolutionary tracks are calculated for various CO dwarf and He-star masses. Consideration is given to the probable type of burning in these systems and the possible relationships between these binaries and SN I and peculiar SNs with H II regions.

Affiliated with

Also associated with

No associations

Rating

Evolution of a binary system consisting of a helium star and a white dwarf does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Evolution of a binary system consisting of a helium star and a white dwarf, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of a binary system consisting of a helium star and a white dwarf will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1560279