On the production of hydrocarbons in Titan's atmosphere

dc.contributor.author	Saxena, P. P
dc.contributor.author	Bhatnagar, S
dc.contributor.author	Singh, M
dc.date.accessioned	2008-05-26T10:58:14Z
dc.date.available	2008-05-26T10:58:14Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 2, pp. 67 - 73	en
dc.identifier.uri	http://hdl.handle.net/2248/2346
dc.description.abstract	The production of C(1 D) atoms and their role in the production of (C1, C2, C3, C4) hydrocarbons in Titan's atmosphere are discussed. The reaction between C(1 D) atom and H2 molecule to produce the methylidyne (CH) radical (Okabe, 1978) is suggested as a possible mechanism which provides an additional route to the production of hydrocarbons in Titan's atmosphere.	en
dc.format.extent	189374 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/2003BASI...31...67S	en
dc.subject	Chemical reactions	en
dc.subject	C(1 D) atoms	en
dc.subject	Titan's atmosphere	en
dc.title	On the production of hydrocarbons in Titan's atmosphere	en
dc.type	Article	en