The early type contact binary system V 382 Cygni

Details The early type contact binary system V 382 Cygni The early type contact binary system V 382 Cygni

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26as..134..327d&link_type=abstract

Astronomy and Astrophysics Supplement, v.134, p.327-331

Astronomy and Astrophysics

Astrophysics

7

Stars: Binaries: Eclipsing, Stars: Individual: V 382 Cyg

Scientific paper

New photometric data set of the early type contact binary V 382 Cyg have been analyzed with emphasis on determining the photometric mass ratio of the system. The result (q=0.68) supports the value given by \cite[Popper & Hill (1991).]{pop91} A study of the system using new data shows a period increase of about 3.28 s per century, which corresponds to a very large rate ~ 5.0 10(-6) {M_sun/yr} of mass transfer from the less massive to the more massive component under the conservative mass transfer hypothesis.

Affiliated with

Also associated with

No associations

Rating

The early type contact binary system V 382 Cygni 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 early type contact binary system V 382 Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The early type contact binary system V 382 Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1184163