On the origin of the Galactic ridge recombination lines.
| 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.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.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.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 |