Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aj....136..337z&link_type=abstract
The Astronomical Journal, Volume 136, Issue 1, pp. 337-343 (2008).
Astronomy and Astrophysics
Astronomy
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.
Qian Sheng Bang
Yang Yuan-Gui
Zhu Li Ying
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