Common envelope evolution of binary stars

Details Common envelope evolution of binary stars Common envelope evolution of binary stars

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ssrv...50..299l&link_type=abstract

(IAU, NSERC, Canadian Institute of Theoretical Astrophysics, et al., Colloquium on Algols, 107th, Sidney, Canada, Aug. 15-19, 19

Astronomy and Astrophysics

Astrophysics

18

Binary Stars, Mass Transfer, Planetary Nebulae, Stellar Evolution, Supernovae, White Dwarf Stars, Elliptical Galaxies, Stellar Mass, Stellar Orbits

Scientific paper

The common envelope phase in the evolution of binary systems is discussed. The problem of the efficiency of energy deposition into envelope ejection is treated in some detail. The implications of common envelope evolution for the shaping of planetary nebulae with close binary nuclei and for double white dwarf systems, considered to be the progenitors of Type I supernovae, are described.

Affiliated with

Also associated with

No associations

Rating

Common envelope evolution of binary stars 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 Common envelope evolution of binary stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Common envelope evolution of binary stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1052495