The Light Curve Variations of The Active Binaries With Hot Subdwarf Component

Simple item page
dc.creatorSipahi, Esin
dc.creatorEvren, Serdar
dc.date2006-07-10
dc.date.accessioned2026-07-07T07:15:37Z
dc.date.available2026-07-07T07:15:37Z
dc.descriptionWe present the light curve variations of the two active binaries with hot subdwarf component. According to the brightness variations outside of the eclipses, the giant components of the systems are chromospherically active stars. The dark and cool active structures on this components cause the variations of the total light of the systems.
dc.descriptionPublished in Proceedings of the 13th Young Scientists' Conference on Astronomy and Space Physics, held in Kyiv, Ukraine, April 25-29, 2006, Eds.: Golovin, A.; Ivashchenko, G.; Simon, A
dc.identifierhttps://arxiv.org/abs/astro-ph/0607183
dc.identifierhttp://arxiv.org/abs/astro-ph/0607183
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/113280
dc.subjectAstrophysics
dc.titleThe Light Curve Variations of The Active Binaries With Hot Subdwarf Component
dc.typetext

Files

Collections

arXiv