The 'mass loss-envelope mass' dependence in eclipsing binaries with emission lines in the spectrum

Details The 'mass loss-envelope mass' dependence in eclipsing binaries with emission lines in the spectrum The 'mass loss-envelope mass' dependence in eclipsing binaries with emission lines in the spectrum

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..659k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, May-June 1987, p. 659-661. In Russian.

Astronomy and Astrophysics

Astronomy

Eclipsing Binary Stars, Emission Spectra, Line Spectra, Stellar Envelopes, Stellar Mass Ejection, Mass Flow Rate, Polarimetry, Spectrum Analysis, Stellar Models, Stellar Winds

Scientific paper

Based upon the data of envelope masses in eclipsing binary stars determined with polarimetric and spectral methods as well as upon those of mass losses calculated from variations in periods of these stars, the dependence "mass loss - envelope mass" has been constructed. The dependence is confirmed by the data on the eclipsing star with an envelope RY Sct.

Affiliated with

Also associated with

No associations

Rating

The 'mass loss-envelope mass' dependence in eclipsing binaries with emission lines in the spectrum 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 'mass loss-envelope mass' dependence in eclipsing binaries with emission lines in the spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 'mass loss-envelope mass' dependence in eclipsing binaries with emission lines in the spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1814306