The First Multi-Color Photometric Study of the Near-Contact Binary as Serpentis

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4

Binaries: Close, Binaries: Eclipsing, Stars: Evolution, Stars: Individual: As Serpentis

Scientific paper

The first complete multi-color CCD photometric light curves of the eclipsing binary AS Ser were obtained over three nights in 2005. Using the latest Wilson-Devinney (WD) code, we computed the photometric elements of this system. It turns out that AS Ser is a near-contact binary system with both components filling more than 99% of their Roche lobes. It belongs to a marginal contact binary system within the parameter uncertainties. The marginal characteristic of AS Ser reveals that this target may be in a rare phase predicted by the thermal relaxation oscillation (TRO) theory. The asymmetry of the light curves can be explained by a dark spot on the secondary component, which is consistent with its late-type nature. Combining all available times of light minimum, we derived a new orbital period of AS Ser and found a periodic oscillation varying within an amplitude of 0.0049 days and a period of 11.8 years. This period change may be the result of the light-time effect due to a presumed tertiary component (M 3 > 0.28M sun) or might result from magnetic activity cycles of the two components.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The First Multi-Color Photometric Study of the Near-Contact Binary as Serpentis 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 The First Multi-Color Photometric Study of the Near-Contact Binary as Serpentis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The First Multi-Color Photometric Study of the Near-Contact Binary as Serpentis will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1137953

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.