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

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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

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