Interstellar shocked region chemistry - certain reactions between interstellar molecules and O and N atoms

dc.contributor.author	Ghosh, K. K
dc.contributor.author	Saleem, S. S
dc.contributor.author	Kutty, K. N
dc.date.accessioned	2008-08-18T06:59:34Z
dc.date.available	2008-08-18T06:59:34Z
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. 293 – 294	en
dc.identifier.uri	http://hdl.handle.net/2248/3160
dc.description	Restricted Access	en
dc.description.abstract	The reactions between O and N atoms and certain interstellar molecules (H/sub2S, NH/sub3, H/sub2CO, CH/sub3OH, C/sub2H/sub5OH) are studied using the dynamical flowing after glow method. It is found that NH and OH radicals are formed which can be used as a diagnostic probe to differentiate between interstellar shocked and heated regions.	en
dc.format.extent	132844 bytes
dc.format.mimetype	application/pdf
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..293G	en
dc.subject	Interstellar molecules	en
dc.title	Interstellar shocked region chemistry - certain reactions between interstellar molecules and O and N atoms	en
dc.type	Article	en