Periodic modulations in the optical light curves of EX Hydrae

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3880

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DC Field	Value	Language
dc.contributor.author	Seetha, S	-
dc.contributor.author	Sharma, D. P	-
dc.contributor.author	Padmini, V. N	-
dc.contributor.author	Marar, T. M. K	-
dc.contributor.author	Kasturirangan, K	-
dc.date.accessioned	2008-09-24T14:41:36Z	-
dc.date.available	2008-09-24T14:41:36Z	-
dc.date.issued	1987-02	-
dc.identifier.citation	Astrophysics and Space Science , Vol. 130, No. 1 - 2, pp. 193 - 196	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/3880	-
dc.description.abstract	The authors present here new results on the periodic modulations in the optical light curves of EX Hydrae observed during 1982 - 84. The period analysis has been done using synchronous summation and discrete Fourier transform methods. The authors report new periodicities at 34.7 min and 26.7 min apart from confirming the detection of 46.3 min modulation recently reported. They also include their data to derive the rate of decrease of the 67 min period.	en
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00654994	en
dc.subject	Accretion disks	en
dc.subject	Eclipsing binary stars	en
dc.subject	Light curve	en
dc.subject	Variable stars	en
dc.subject	White dwarf stars	en
dc.subject	Fourier transformation	en
dc.subject	Red dwarf stars	en
dc.title	Periodic modulations in the optical light curves of EX Hydrae	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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