The Solar-Type Contact Binary BX Pegasi Revisited
Jae Woo Lee, Seung-Lee Kim, Chung-Uk Lee, and Jae-Hyuck Youn

TL;DR
This study provides new photometric observations of the contact binary BX Peg, revealing magnetic activity, brightness disturbances, and complex period variations including potential additional companions or magnetic cycles.
Contribution
It offers the first detailed analysis of short-term brightness disturbances and models magnetic activity effects with updated period change insights for BX Peg.
Findings
Brightness disturbances linked to magnetic activity modeled with star spots.
Complex period variations include secular decrease and possible third or fourth companions.
Short-term oscillations suggest additional bodies or magnetic cycles.
Abstract
We present the results of new CCD photometry for the contact binary BX Peg, made during three successive months beginning on September 2008. As do historical light curves, our observations display an O'Connell effect and the November data by themselves indicate clear evidence for very short-time brightness disturbance. For these variations, model spots are applied separately to the two data set of Group I (Sep.--Oct.) and Group II (Nov.). The former is described by a single cool spot on the secondary photosphere and the latter by a two-spot model with a cool spot on the cool star and a hot one on either star. These are generalized manifestations of the magnetic activity of the binary system. Twenty light-curve timings calculated from Wilson-Devinney code were used for a period study, together with all other minimum epochs. The complex period changes of BX Peg can be sorted into a…
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