Near infrared high angular resolution observations of stars and circumstellar regions by the technique of lunar occultations

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1540

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DC Field	Value	Language
dc.contributor.author	Chandrasekhar, T	-
dc.contributor.author	Ashok, N. M	-
dc.contributor.author	Sam Ragland	-
dc.date.accessioned	2007-05-07T07:41:55Z	-
dc.date.available	2007-05-07T07:41:55Z	-
dc.date.issued	1993	-
dc.identifier.citation	BASI, Vol. 21, pp. 499-501	en
dc.identifier.uri	http://hdl.handle.net/2248/1540	-
dc.description.abstract	A program of high angular resolution observations of stars and their circumstellar regions using the technique of lunar occultations has been initiated at the Physical Research Laboratory, Ahmedabad. A liquid nitrogen cooled InSb detector based high speed infrared photometer with millisecond data acquisition capabilities has been developed and a dozen occultations have been successfully observed at 2.2 micrometers. A detailed analysis of the system capability suggests a presently achievable angular resolution of 3.5 milliarcseconds.	en
dc.format.extent	139978 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Near infrared	en
dc.subject	Lunar occultation	en
dc.title	Near infrared high angular resolution observations of stars and circumstellar regions by the technique of lunar occultations	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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