Mass loss and shell masses of close binary stars

Details Mass loss and shell masses of close binary stars Mass loss and shell masses of close binary stars

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.131..675k&link_type=abstract

(IAU, Colloquium on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, 93rd, Bamberg, West

Statistics

Computation

2

Eclipsing Binary Stars, Mass Transfer, Orbital Elements, Stellar Envelopes, Stellar Mass Ejection, Cataclysmic Variables, Computational Astrophysics, Mass Flow Rate, Stellar Mass Accretion

Scientific paper

The values of period changes for six eclipsing binaries with powerful circumstellar envelopes are used to determine mass transfer rates. From comparison of mass transfer rates and shell mass values, an expression is derived which describes the initial character of the outflow of matter, allowing the determination of the time interval of the shell-matter substitution. A mass transfer rate of 3 x 10 to the 20 g/s is derived for the system RY Sct. It is concluded that a certain amount of matter accumulates in the nearby regions of the system for certain mass transfer rates.

Affiliated with

Also associated with

No associations

Rating

Mass loss and shell masses of close 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 Mass loss and shell masses of close binary stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass loss and shell masses of close binary stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1452615