Photometry of EX Hya

dc.contributor.author	Shylaja, B. S
dc.date.accessioned	2005-08-27T04:40:09Z
dc.date.available	2005-08-27T04:40:09Z
dc.date.issued	1985-04
dc.identifier.citation	Astrophysics and Space Science. Vol. 111, No. 2, pp. 407 – 411	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/577
dc.description.abstract	Photometric observations of EX Hya in B and V filters are reported. The 67 min modulation of the light curve is also found to be in good agreement with the results of earlier studies. The (B-V) colour variation with respect to the 67 min variation is found to be opposite to those of typical colour variation during hump/superhump activity in other dwarf novae. The model of an intermediate polar is discussed.
dc.format.extent	7229 bytes
dc.format.mimetype	text/html
dc.language.iso	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1985Ap%26SS.111..407S
dc.relation.uri	http://dx.doi.org/10.1007/BF00649980
dc.subject	Cataclysmic Variables
dc.subject	Dwarf Novae
dc.subject	Light Curve
dc.subject	Stellar Color
dc.subject	Stellar Spectrophotometry
dc.subject	Stellar Models
dc.subject	White Dwarf Stars
dc.title	Photometry of EX Hya	en
dc.type	Article	en