Possible change of the orbital period of the nova-like binary V Sagittae.

Details Possible change of the orbital period of the nova-like binary V Sagittae. Possible change of the orbital period of the nova-like binary V Sagittae.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...309..775s&link_type=abstract

Astronomy and Astrophysics, v.309, p.775-776

Astronomy and Astrophysics

Astrophysics

6

Binaries: Eclipsing, Circumstellar Matter, Novae, Cataclysmic Variables, Stars: Individual: V Sge

Scientific paper

Analysis of the available minimum timings of this cataclysmic binary
spanning 31 years revealed fairly stable orbital period. The parabolic
course leads to very small {DELTA}P/P=-2.94x10^-10^.

Affiliated with

Also associated with

No associations

Rating

Possible change of the orbital period of the nova-like binary V Sagittae. 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 Possible change of the orbital period of the nova-like binary V Sagittae., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possible change of the orbital period of the nova-like binary V Sagittae. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1351324