Interacting binary stars - Freaks or rosetta stones

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

13

Eclipsing Binary Stars, Stellar Evolution, Stellar Mass Accretion, Stellar Mass Ejection, Abundance, Light Curve, Stellar Envelopes, Stellar Spectra, Stellar Winds, Variable Stars

Scientific paper

Attention is given to semidetached binaries of the Algol type and to related interacting systems, such as Beta Lyrae and the W Serpentis stars. A brief description is given of observational problems. The basic properties of the Algol variables are satisfactorily explained by means of evolutionary models that assume considerable mass transfer between the components. It is pointed out that ultraviolet spectra obtained with the IUE satellite corroborate the view that the present subgiant secondary component was initially the more massive star and that it has been stripped of a large fraction of its mass so that the deep layers affected by CNO processing are now denuded. It is believed that the present-day 'classical' Algols must have undergone a phase of rapid mass transfer in the past and that Beta Lyrae and the W Serpentis stars are probably closer to that stage than ordinary Algols. Around the accreting star a complex structure is formed, and an induced stellar wind may blow a large part of the transferred matter out of the system.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Interacting binary stars - Freaks or rosetta stones 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 Interacting binary stars - Freaks or rosetta stones, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interacting binary stars - Freaks or rosetta stones will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1803926

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.