XX Cam -The Inactive R CrB Star

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DC Field	Value	Language
dc.contributor.author	Kameswara Rao, N	-
dc.contributor.author	Ashok, N. M	-
dc.contributor.author	Kulkarni, P. V	-
dc.date.accessioned	2009-01-02T11:19:16Z	-
dc.date.available	2009-01-02T11:19:16Z	-
dc.date.issued	1980-09	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 1, pp. 71 - 78	en
dc.identifier.issn	0250- 6335	-
dc.identifier.uri	http://hdl.handle.net/2248/4233	-
dc.description.abstract	Infrared observations obtained six years apart of the R CrB type star XX Cam do not show any infrared excess, unlike all other members of the class. The observed colours match a 7000 K black body energy distribution quite well. From the year 1898 till todate, apparently XX Cam has undergone only one visual light minimum in 1940. The lack of infrared excess, the abundance peculiarities and further lack of small amplitude light variations with periods of a few tens of days, which are characteristic of R CrB type stars, are discussed in terms of theoretical pulsation models of helium stars.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1980JApA....1...71K	en
dc.rights	© Indian Academy of Sciences	en
dc.subject	R Crb Stars	en
dc.subject	Infrared Excess	en
dc.title	XX Cam -The Inactive R CrB Star	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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