Photometric period variation of V 1379 Aql


Sipahi E. , Evren S., Tas C., İbanoğlu C.

BALTIC ASTRONOMY, vol.15, no.2, pp.199-205, 2006 (Journal Indexed in SCI) identifier identifier

  • Publication Type: Article / Article
  • Volume: 15 Issue: 2
  • Publication Date: 2006
  • Title of Journal : BALTIC ASTRONOMY
  • Page Numbers: pp.199-205

Abstract

V 1379 Aql is an eclipsing binary consisting a hot subdwarf (sdB) and a red giant star (K0III/IV). According to the brightness variation outside of eclipses, the giant component is a chromospherically active star. The dark and cool active structures on this component and their evolution cause the variation of the total light of the system. Photometric observations spanning 16 years yield the variations of the photometric period and the mean brightness. There is a correlation between them. We suggest that the photometric period decreases as the latitude of the active region moves toward the equator.