On the origin of the Galactic ridge recombination lines.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1085

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DC Field	Value	Language
dc.contributor.author	Anantharamaiah, K.R.	-
dc.date.accessioned	2006-01-04T10:54:05Z	-
dc.date.available	2006-01-04T10:54:05Z	-
dc.date.issued	1986	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1986, Vol. 7, p131-139.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/1085	-
dc.description.abstract	Radio recombination lines are known to be observable at positions along the galactic ridge which are free of discrete continuum sources. Based on the results of a recent survey of H272 alpha lines it is shown that most of the observed Galactic ridge recombination lines can be explained as emission from outer low-density envelopes of normal H II regions. The distribution of low-density ionized gas and discrete H II regions as a function of the distance from the Galactic center is also derived.	en
dc.format.extent	945695 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	Galaxy	en
dc.subject	Recombination Lines	en
dc.subject	Galactic ridge	en
dc.subject	H2 regions	en
dc.subject	Low density envelops	en
dc.subject	Distribution	en
dc.title	On the origin of the Galactic ridge recombination lines.	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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