Mass transfer in TV Cassiopeiae

Details Mass transfer in TV Cassiopeiae Mass transfer in TV Cassiopeiae

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..63..247c&link_type=abstract

Astrophysics and Space Science, vol. 63, no. 1, June 1979, p. 247-252.

Astronomy and Astrophysics

Astrophysics

4

Binary Stars, Cassiopeia Constellation, Mass Transfer, Stellar Mass Ejection, Variable Stars, Astrophysics, Dynamic Stability, Periodic Variations

Scientific paper

The period variations of TV Cassiopeiae between 1901 and 1977 are discussed in the light of the period-change model proposed by Biermann and Hall (1973). During each period decrease 4.0 millionths of a solar mass is transferred from the secondary star to the primary. The average observable mass-transfer rate is found to be 430 billionths of a solar mass per year. This average rate corresponds to the thermal time scale of the mass-losing star.

Affiliated with

Also associated with

No associations

Rating

Mass transfer in TV Cassiopeiae 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 transfer in TV Cassiopeiae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass transfer in TV Cassiopeiae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1775529