Light variation of the delta Scuti star 38 CNC

dc.contributor.author	Gupta, S. K.
dc.date.accessioned	2011-07-25T09:19:35Z
dc.date.available	2011-07-25T09:19:35Z
dc.date.issued	1979
dc.identifier.uri	http://hdl.handle.net/123456789/826
dc.description.abstract	The light curves of the δ Scuti variable 38 Cnc, which is member of the Praesepe cluster, have been analysed using the techniques of perodogram analysis and least square solutions. The star pulsates in the second overtone as well as in the first overtone modes with the periods of 0. ͩ 10229 and 0. ͩ 12715 respectively. The period ratio of the second overtone to first overtone indicates that the star pulsates in the radial mode. The absolute magnitude, derived from the cluster modulus, in 0. ͫ 52. The effective temperature and mass of the star are derived to be nearly 7800⁰K and 2.2M ʘ respectively.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	basi7-72
dc.subject	Delta Scuti Star 38 CNC	en_US
dc.title	Light variation of the delta Scuti star 38 CNC	en_US
dc.type	Article	en_US