Photometry of HU Tauri

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4138

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DC Field	Value	Language
dc.contributor.author	Parthasarathy, M	-
dc.contributor.author	Sarma, M. B. K	-
dc.date.accessioned	2008-12-19T10:43:15Z	-
dc.date.available	2008-12-19T10:43:15Z	-
dc.date.issued	1980-10	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 72, No. 2, pp. 477 - 496	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/4138	-
dc.description.abstract	Photoelectric observations of the bright eclipsing binary system HU Tauri are presented. The observations were made with standardB andV filters. Observations made during the eclipses yielded six epochs of minimum light. A study of all the available times of minimum light has been made. Analysis of all the photoelectric times of minimum light yielded the following new ephemeris: JD 2441275.3166 +2 . d 0563107E. Asymmetries in the light curves of HU Tauri were noticed.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1980Ap%26SS..72..477P	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00639151	en
dc.title	Photometry of HU Tauri	en
dc.type	Article	en
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