Light curve analyses of new eclipsing binary systems with eccentric orbits

Details Light curve analyses of new eclipsing binary systems with eccentric orbits Light curve analyses of new eclipsing binary systems with eccentric orbits

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008newa...13..252b&link_type=abstract

New Astronomy, Volume 13, Issue 4, p. 252-254.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

A photometric study of seven new eclipsing binary systems with eccentric orbits, namely, V466 Car, V493 Car, V529 Car, MN TrA, V398 Lac, V402 Lac and V821 Cas, is presented. The photometric data analyzed were taken from the Hipparcos database. The secondary minima in all systems were shifted by different amounts from the phase 0.5 giving clear evidence of their eccentric orbits. The EBOP computer program based upon models by Nelson et al. [Popper, D.M., Etzel, P.E., 1981. AJ 86, 102] was used in the analysis of the photometric data to deduce the orbital geometry in space and the relative sizes and luminosities of the component stars.

Affiliated with

Also associated with

No associations

Rating

Light curve analyses of new eclipsing binary systems with eccentric orbits 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 Light curve analyses of new eclipsing binary systems with eccentric orbits, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Light curve analyses of new eclipsing binary systems with eccentric orbits will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1075432