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The interstellar clouds of Adams and Blaauw revisited: An HI absorption study - I

dc.contributor.authorRajagopal, Jayadev
dc.contributor.authorSrinivasan, G
dc.contributor.authorDwarakanath, K S
dc.date.accessioned2006-01-02T08:54:45Z
dc.date.available2006-01-02T08:54:45Z
dc.date.issued1998
dc.description.abstractThis investigation is aimed at clarifying the nature of the interstellar gas seen in absorption against bright O and B stars. Towards this end we have obtained for the first time HI absorption spectra towards radio sources very close to the lines of sight towards twenty five bright stars previously studied. In this paper we describe the selection criteria, the details regarding our observations, and finally present the absorption spectra. In the accompanying paper we analyse the results and draw conclusions.en
dc.format.extent1512441 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationJournal of Astrophysics and Astronomy, 1998, Vol. 19, p97-116.en
dc.identifier.issn0250-6335
dc.identifier.urihttp://hdl.handle.net/2289/1034
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.subjectISM: clouds, structureen
dc.subjectRadio lines: ISMen
dc.titleThe interstellar clouds of Adams and Blaauw revisited: An HI absorption study - Ien
dc.typeArticleen

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