Probability for the formation of complex ring molecules in interstellar medium and their detection proposal

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4259

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DC Field	Value	Language
dc.contributor.author	Ghosh, K. K	-
dc.date.accessioned	2009-01-09T15:07:33Z	-
dc.date.available	2009-01-09T15:07:33Z	-
dc.date.issued	1987	-
dc.identifier.citation	M. S. Vardya and S. P. Tarafdar., eds., Astrochemistry, Proceedings of the 120th symposium of the International Astronomical Union held at Goa, December 3 – 7, 1985, pp. 253 – 254	en
dc.identifier.uri	http://hdl.handle.net/2248/4259	-
dc.description.abstract	The pathways for the formation and destruction processes of ring molecules in the interstellar medium are proposed and their abundances are calculated under steady state conditions. The calculated abundances are of the order of 10/sup-12n(H), where n(H) is the abundance of hydrogen. A detection proposal is presented.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.ispartofseries	International Astronomical Union Symposium No. 120	-
dc.relation.uri	http://adsabs.harvard.edu/abs/1987IAUS..120..253G	en
dc.subject	Interstellar medium	en
dc.title	Probability for the formation of complex ring molecules in interstellar medium and their detection proposal	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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