Period study of GH Pegasi

dc.contributor.author	Srivastava, R. K.
dc.date.accessioned	2010-02-24T05:11:35Z
dc.date.available	2010-02-24T05:11:35Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/571
dc.description.abstract	The period study of the eclipsing binary system GH Pegasi has been presented for the first time. A new period (p=2.ͩ 556135) of GH Peg, based on all available times of minima, has been given, O-C diagrams of the system have also been presented for the first time, and the period changes present in the system have been analysed. The period shows changes around the years 1972 and 1981. The total period change in different portions of the O-C diagram, based on the corrected period, ranges from 5.2x10⁻⁶d to 7.0x10⁻⁵d. The photoelectric minima show sufficient large scatter in the system.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass134-177
dc.subject	Eclipsing binary system - GH Pegasi	en_US
dc.title	Period study of GH Pegasi	en_US
dc.type	Article	en_US