High Rydberg state carbon recombination lines from interstellar clouds

Anantharamaiah, K.R.; Kantharia, N.G.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2552

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DC Field	Value	Language
dc.contributor.author	Anantharamaiah, K.R.	-
dc.contributor.author	Kantharia, N.G.	-
dc.date.accessioned	2007-06-01T06:23:05Z	-
dc.date.available	2007-06-01T06:23:05Z	-
dc.date.issued	1999	-
dc.identifier.citation	New Perspectives on the Interstellar Medium, ASP Conference Series Vol.168, p197, 1999.	en
dc.identifier.isbn	1-886733-89-9	-
dc.identifier.uri	http://hdl.handle.net/2289/2552	-
dc.description	Restricted Access. An open access version is available at NASA ADS. New Perspectives on the Interstellar Medium, ASP Conference Series 168, Eds. A. R. Taylor, T. L. Landecker, and G. Joncas. Astronomical Society of the Pacific (San Francisco), 1999.	en
dc.description.abstract	We report observations of carbon recombination lines near 34.5 MHz (qunatum number n=578) and 325 MHz (n=272) made towards Cas A, the Galactic centre and about ten other directions in the galactic plane. Constraints on the physical conditions in the line forming regions are derived from these and other existing observations. The CII regions that produce the low-frequency lines are most likely associated with the neutral HI component of the ISM.	en
dc.format.extent	385653 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1999ASPC..168..197A	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/9903076	en
dc.rights	1999 Astronomical Society of the Pacific	en
dc.title	High Rydberg state carbon recombination lines from interstellar clouds	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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