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dc.contributor.author Srivastava, R. K.
dc.date.accessioned 2010-02-15T06:27:08Z
dc.date.available 2010-02-15T06:27:08Z
dc.date.issued 1989
dc.identifier.citation This article downloded from ADS Free Online Journal en_US
dc.identifier.uri http://hdl.handle.net/123456789/515
dc.description.abstract A detailed study of the eclipsing binary system AW UMa is presented. A new period (P = 0.ᵈ4387317) is given. Period changes in different portions of the O-C diagram, based on new period, have been estimated. The total change in period (ΔP) ranges from 2.2х10¯⁷ to 2.8х10¯⁶d, which is normal for AW UMa systems. Two distinct linear trends of period are visible in the O-C diagram. A third trend shows a new change in the period behaviour, which is yet to be confirmed. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries ass154-179
dc.subject AW UMa en_US
dc.title Period study of AW UMa en_US
dc.type Article en_US


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