A light and period study of SV Camelopardalis

Details A light and period study of SV Camelopardalis A light and period study of SV Camelopardalis

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...376..158a&link_type=abstract

Astronomy and Astrophysics, v.376, p.158-164 (2001)

Astronomy and Astrophysics

Astrophysics

15

Stars: Binaries: Eclipsing, Stars: Individual: Sv Cam

Scientific paper

New BVR light curves and times of minimum light for the short period RS CVn system SV Cam were analysed to derive the physical parameters of the system and the parameters of the third body orbit. The light curves obtained at the TÜBITAK National Observatory during two nights in 2000 show considerable asymmetry and night-to-night variations. The analysis of the light curves is made using Djurasevic's inverse problem method. The Roche model with spotted areas on the hotter primary component yields a good fit to observations. The extensive series of published photoelectric minima times indicate that the eclipsing pair orbits around the common mass center of the triple system with a period of 41.32 yr. Table 1 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/376/158

Affiliated with

Also associated with

No associations

Rating

A light and period study of SV Camelopardalis 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 light and period study of SV Camelopardalis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A light and period study of SV Camelopardalis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1483535