Identification of emission bands in P/Halley

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4647

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DC Field	Value	Language
dc.contributor.author	Bhattacharyya, J. C	-
dc.contributor.author	Babu, G. S. D	-
dc.contributor.author	Ghosh, K. K	-
dc.contributor.author	Jayakumar, K	-
dc.contributor.author	Appakutty, M	-
dc.date.accessioned	2009-07-16T13:42:50Z	-
dc.date.available	2009-07-16T13:42:50Z	-
dc.date.issued	1986	-
dc.identifier.citation	Current Science, Vol. 55, No. 16, pp. 761 - 764	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2248/4647	-
dc.description.abstract	Spectrophotometric studies of P /Halley (r = 1.98 AU, Δ= 1.19AU, r = 1.97, Δ = 1.16 AU and r = 1.95 AU, Δ. = 1.13 AU) in the spectral range 3900 A - 6450 A were made on three nights and identifications of emission features include: CO/sup+, C/sub3 , C/sub2 , CN, CH, NH/sub2 , H/sub3 , NaI, 0I and H/sub2O/sup+ molecules. For the first time H/sub3 molecule has been found in cometary atmospheres. Certain strong emission bands have been found in the spectra of P /Halley which are yet to be identified.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://www.ias.ac.in/j_archive/currsci/volindex.html	en
dc.subject	Comet 1910 II Halley	en
dc.title	Identification of emission bands in P/Halley	en
dc.type	Article	en
Appears in Collections:	IIAP Publications J.C.Bhattacharyya (1982 - 1990)

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