Auto-correlation of Binary stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4984

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DC Field	Value	Language
dc.contributor.author	Saha, S. K	-
dc.contributor.author	Maitra, D	-
dc.date.accessioned	2010-01-16T12:04:18Z	-
dc.date.available	2010-01-16T12:04:18Z	-
dc.date.issued	2001	-
dc.identifier.citation	Indian Journal of Physics, Vol. 75B, pp. 391 - 398	en
dc.identifier.issn	1625-1776	-
dc.identifier.uri	http://hdl.handle.net/2248/4984	-
dc.description.abstract	Speckle interferometric technique is used to record a series of short exposure images of several close binary stars with sub-arcsecond separation through a narrow band filter centred at H$\alpha$ at the Cassegrain focus of the 2.34 meter Vainu Bappu telescope (VBT), situated at Vainu Bappu Observatory (VBO), Kavalur. The auto-correlation method is developed under Image Reduction Analysis Facility (IRAF). Wiener filter is included in the programme to eliminate spurious high frequency contributions; a few sets of data provide the optimised results. The auto-correlated image of these stars gives the separation of the binary components.	en
dc.language.iso	en	en
dc.publisher	Indian Association for the Cultivation of Science	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0106119	en
dc.rights	© Indian Association for the Cultivation of Science	en
dc.subject	Speckle Imaging	en
dc.subject	Auto-Correction	en
dc.subject	Binary Stars	en
dc.title	Auto-correlation of Binary stars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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