Emission from the head of comet P/Halley during post-perihelion

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1831

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DC Field	Value	Language
dc.contributor.author	Goraya, P. S	-
dc.contributor.author	Rautela, B. S	-
dc.contributor.author	Sanwal, B. B	-
dc.contributor.author	Pandey, A. K	-
dc.contributor.author	Duggal, H. K	-
dc.date.accessioned	2007-09-26T11:26:45Z	-
dc.date.available	2007-09-26T11:26:45Z	-
dc.date.issued	1996	-
dc.identifier.citation	BASI, Vol.24 No. 4 pp. 649-652	en
dc.identifier.uri	http://hdl.handle.net/2248/1831	-
dc.description.abstract	Spectral scans of the head of periodic comet Halley (1982i)covering the wavelength range λλ 320 - 700 nm, are presented for five nights during the months of April an May, 1986. These observations were made when the heliocentric distance of the comet varied from 1.57 - 1.82 AU. Bright emissison features due to CN band at λ 388 nm (ΔV = 0), CH + C3 band at λ 405 nm (ΔV = 0 )and Swan band sequence of C2 at λ 474 nm (ΔV = + 1), λ 516 nm (ΔV = 0)an λ 564 nm (ΔV = -1)have been identified. The fluxes at each emission bands have been measured	en
dc.format.extent	224603 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996BASI...24..649G	en
dc.subject	Comet - molecular emissions	en
dc.title	Emission from the head of comet P/Halley during post-perihelion	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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