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

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