3.0 to 3.5 micron spectrum of V 348 SGR and R CrB

dc.contributor.author	Nandy, K
dc.contributor.author	Kameswara Rao, N
dc.contributor.author	Morgan, D. H
dc.date.accessioned	2009-03-03T09:29:39Z
dc.date.available	2009-03-03T09:29:39Z
dc.date.issued	1986
dc.identifier.citation	Kurt Hunger, Detlef Schoenberner, and N. Kameswara Rao., eds., Hydrogen Deficient Stars and Related Objects, Proceedings of IAU Colloq. 87, held in Mysore, India, Nov. 10 - 15, 1985, Vol. 128, pp. 203 - 205	en
dc.identifier.uri	http://hdl.handle.net/2248/4367
dc.description.abstract	With a view to search for weaker dust spectral features the authors obtained the spectrum of R CrB and V348 Sgr with higher resolution than employed before.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co	en
dc.relation.ispartofseries	IAU Colloquium No. 128
dc.relation.uri	http://adsabs.harvard.edu/abs/1986hdsr.proc..203N	en
dc.subject	Micron Spectrum	en
dc.subject	V 348 SGR	en
dc.title	3.0 to 3.5 micron spectrum of V 348 SGR and R CrB	en
dc.type	Article	en