A synchronism parameter for binary stars

Details A synchronism parameter for binary stars A synchronism parameter for binary stars

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cha%26a..22..245l&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 22, Issue 2, p. 245-245.

Astronomy and Astrophysics

Astrophysics

Scientific paper

A synchronism parameter is defined by the ratio of the theoretical
apsidal period presuming synchronism to the observed period. As judged
by this parameter, Y Cyg is a nearly synchronous binary, and CW Cep, a
synchronous one,-in agreement with previous authors.

Affiliated with

Also associated with

No associations

Rating

A synchronism parameter for 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 A synchronism parameter for binary stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A synchronism parameter for binary stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1224573