Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5299
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dc.contributor.authorParvathi, V. S-
dc.contributor.authorSofia, U. J-
dc.contributor.authorMurthy, J-
dc.contributor.authorBabu, B. R. S-
dc.date.accessioned2011-01-13T10:26:42Z-
dc.date.available2011-01-13T10:26:42Z-
dc.date.issued2010-09-
dc.identifier.citationBASI, Vol. 38, No. 2&3, pp. 93-101en
dc.identifier.urihttp://hdl.handle.net/2248/5299-
dc.description.abstractWe present interstellar CII (1334.5323 \AA) and CII* (1335.7077 \AA) column density measurements along 14 Galactic sight-lines. These sight-lines sample a variety of Galactic disk environments and include paths that range nearly two orders of magnitude in average hydrogen densities (<n(H)>) along the lines of sight. Five of the sight-lines show super-Solar gas phase abundances of carbon. Our results show that the excess carbon along these sight-lines may result from different mechanisms taking place in the regions associated with these stars.en
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://www.ncra.tifr.res.in/~basi/10JuneSep/Abstracts/380932010.htmen
dc.rights© Astronomical Society of Indiaen
dc.subjectLine: profiles -- ISMen
dc.subjectClouds -- ISMen
dc.subjectAbundances -- ultraviolet: ISMen
dc.titleEstimation of CII and CII* column densities along Galactic sight-linesen
dc.typeArticleen
Appears in Collections:BASI Publications
IIAP Publications

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