The Thermal Evolution of Mass Losing Donors in AM CVn Binary Systems

Details The Thermal Evolution of Mass Losing Donors in AM CVn Binary Systems The Thermal Evolution of Mass Losing Donors in AM CVn Binary Systems

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..404..241t&link_type=abstract

The Eighth Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series, Vol. 404, proceed

Astronomy and Astrophysics

Astrophysics

Scientific paper

The thermal evolution of arbitrarily degenerate stellar models for the mass losing component in AM CVn binary systems formed through the white dwarf evolutionary channel is investigated for a range of initial orbital periods and initial system masses. Based on these models, the evolutionary phases and properties of AM CVn binary systems are described and the observational signature of their donors is discussed.

Affiliated with

Also associated with

No associations

Rating

The Thermal Evolution of Mass Losing Donors in AM CVn Binary Systems 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 The Thermal Evolution of Mass Losing Donors in AM CVn Binary Systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Thermal Evolution of Mass Losing Donors in AM CVn Binary Systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-818612