Probing circumstellar dust formation through high resolution spectroscopy

dc.contributor.author	Kameswara Rao, N
dc.date.accessioned	2006-03-14T10:12:28Z
dc.date.available	2006-03-14T10:12:28Z
dc.date.issued	2005-06
dc.identifier.citation	BASI, Vol. 33, No. 2, pp. 159-165	en
dc.identifier.uri	http://hdl.handle.net/2248/766
dc.description.abstract	The existence of cool regions where dust can condense is explored in RCB stars at minimum	en
dc.format.extent	217897 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	RCB stars	en
dc.subject	dust condensation	en
dc.subject	C2 molecule	en
dc.title	Probing circumstellar dust formation through high resolution spectroscopy	en
dc.type	Article	en