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DC Field | Value | Language |
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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) |
Files in This Item:
File | Description | Size | Format | |
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1986_JAA_V7_p131-139.pdf | 9p. | 923.53 kB | Adobe PDF | View/Open |
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