Empirical P-L-C relations for Delta Scuti stars

dc.contributor.author	Gupta, S. K.
dc.date.accessioned	2011-11-11T05:17:30Z
dc.date.available	2011-11-11T05:17:30Z
dc.date.issued	1978
dc.identifier.citation	This article is downloaded from ADS article service	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/859
dc.description.abstract	Separate P-L-C relations have been empirically derived by sampling the δ Scuti stars according to their pulsation modes. The results based on these relations have been compared with those estimated from the model based P-L-C relations and the other existing empirical P-L-C relations. It is found that a separate P-L-C relation for each pulsation mode provides a better correspondence with observations.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass59-85
dc.subject	Delta Scuti Stars, P-L-C relations	en_US
dc.title	Empirical P-L-C relations for Delta Scuti stars	en_US
dc.type	Article	en_US