Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr

Details Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009newa...14..604b&link_type=abstract

New Astronomy, Volume 14, Issue 7, p. 604-606.

Astronomy and Astrophysics

Astronomy

Scientific paper

The apsidal motion analysis of the eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr have been presented. The method described by Lacy (1992) [Lacy, C.H S., 1992. AJ 104, 2213] has been used for the apsidal motion analysis. The apsidal motion periods have been found to be 174.2 ± 1.4, 277.3 ± 21.3 and 7195 ± 174 years for V397 Cep, V493 Car and BW Aqr, respectively.

Affiliated with

Also associated with

No associations

Rating

Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr 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 Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1427499