Period study of IT Persei

dc.contributor.author	Srivastava, R. K.
dc.date.accessioned	2010-02-02T06:41:45Z
dc.date.available	2010-02-02T06:41:45Z
dc.date.issued	1990
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/482
dc.description.abstract	A new period (P = 1.ᵈ533731) of the eclipsing binary system IT Persei has been given, which is based on all available times of minima. O-C diagrams of IT Persai, based on the period given in PPEN (1980) and based on the new period, have been given. Long-term period changes are not present in the system, however, some period fluctuations of the order of 10¯⁵ d are seen around the years 1907, 1921, and 1933.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass166-171
dc.subject	IT Persei	en_US
dc.title	Period study of IT Persei	en_US
dc.type	Article	en_US