Photometric Study of HD224085

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4148

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DC Field	Value	Language
dc.contributor.author	Raveendran, A. V	-
dc.contributor.author	Mohin, S	-
dc.contributor.author	Mekkaden, M. V	-
dc.date.accessioned	2008-12-19T14:42:49Z	-
dc.date.available	2008-12-19T14:42:49Z	-
dc.date.issued	1981-07	-
dc.identifier.citation	Monthly Notices Royal Astronomical Society, Vol. 196, pp. 289 - 296	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2248/4148	-
dc.description.abstract	B and V photometry of HD 224085 obtained on 21 nights between 1979 November and 1980 February is presented. The amplitudes of light variation observed are ~ 0.15mag in both B and V. The photometric period is found to be P/sub phot = 6.7026 ± 0.0034 day. A new orbital solution obtained from the available radial velocity data shows that the orbit period is 6.724464 day. The radius of the visible primary estimated from the Barnes Evens surface brightness relation is ~ 1.9 R, indicating a position above the main sequence.	en
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1981MNRAS.196..289R	en
dc.title	Photometric Study of HD224085	en
dc.type	Article	en
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