On the variability of the suspected beta cephei stars V351, V356, V357 Per

dc.contributor.author	Mahra, H. S.
dc.contributor.author	Mohan, V.
dc.date.accessioned	2011-08-02T04:23:41Z
dc.date.available	2011-08-02T04:23:41Z
dc.date.issued	1979
dc.identifier.uri	http://hdl.handle.net/123456789/828
dc.description.abstract	Hill (1967) has listed a number of suspected Beta Cephei stars. Out of these the stars V351 Per (HD 13051), V356 Per (BD 56°473) and V357 Per (HD 13866) were put on our observing programme, in order to determine their variability.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs1698
dc.subject	Beta cephei	en_US
dc.title	On the variability of the suspected beta cephei stars V351, V356, V357 Per	en_US
dc.type	Article	en_US