Light Variation of the Delta Scuti Star 38 CNC

dc.contributor.author	Gupta, S. K
dc.date.accessioned	2005-08-13T07:09:13Z
dc.date.available	2005-08-13T07:09:13Z
dc.date.issued	1979-09
dc.identifier.citation	BASI, Vol. 7, No. 3, pp. 72-77	en
dc.identifier.uri	http://hdl.handle.net/2248/540
dc.description.abstract	The light curves of the delta Scuti star variable 38 Cnc, which is a member of the Praesepe cluster, have been analysed using the techniques of periodogram 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.d10229 and 0.d12715 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 modules, is 0.m52. The effective temperature and mass of the star are derived to be nearly 7800/sup0/K and 2.2 M respectively.	en
dc.format.extent	659399 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Light Variation	en
dc.subject	Scuti Star	en
dc.title	Light Variation of the Delta Scuti Star 38 CNC	en
dc.type	Article	en