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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1034

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DC Field	Value	Language
dc.contributor.author	Rajagopal, Jayadev	-
dc.contributor.author	Srinivasan, G.	-
dc.contributor.author	Dwarakanath, K.S.	-
dc.date.accessioned	2006-01-02T08:54:45Z	-
dc.date.available	2006-01-02T08:54:45Z	-
dc.date.issued	1998	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1998, Vol. 19, p97-116.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/1034	-
dc.description.abstract	This 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.extent	1512441 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	ISM: clouds, structure	en
dc.subject	Radio lines: ISM	en
dc.title	The interstellar clouds of Adams and Blaauw revisited: An HI absorption study - I	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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