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http://hdl.handle.net/2248/3778
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DC Field | Value | Language |
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dc.contributor.author | Deshpande, A. A | - |
dc.contributor.author | Sastry, Ch. V | - |
dc.date.accessioned | 2008-09-22T16:07:35Z | - |
dc.date.available | 2008-09-22T16:07:35Z | - |
dc.date.issued | 1986-05 | - |
dc.identifier.citation | Astronomy and Astrophysics, Vol. 160, No. 1, pp. 129 - 139 | en |
dc.identifier.issn | 0004-6361 | - |
dc.identifier.uri | http://hdl.handle.net/2248/3778 | - |
dc.description.abstract | Radio continuum absorption observations at 34.5 MHz with a spatial resolution of 34 x 48 arcmin have been obtained for the giant H II region complex W 51 with the decameter-wave radio telescope at Gauribidanur, India (13 deg 36 min N and long 77 deg 27 min E). A mean electron temperature of 9500 + or - 600 K and a background temperature of 28,000 + or - 2600 K have been derived. The proportion of nonthermal emission originating on the near side of W51 corresponds to a mean emissivity of 2 K/pc. The present observations also indicate that the ring towards the east of the nebula (W 51 C) is nonthermal. | en |
dc.language.iso | en | en |
dc.publisher | European Southern Observatory | en |
dc.relation.uri | http://ads.ari.uni-heidelberg.de/abs/1986A%26A...160..129D | en |
dc.subject | H II Regions | en |
dc.subject | Radio Sources (Astronomy) | en |
dc.subject | Supernova Remnants | en |
dc.subject | Decametric Waves | en |
dc.subject | Galactic Radiation | en |
dc.subject | Nonthermal Radiation | en |
dc.subject | Radio Spectroscopy | en |
dc.title | Observations of the giant H II region complex W51 at decameter wavelengths | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Observations of the giant H II region complex W51 at decameter wavelengths | 499.9 kB | Adobe PDF | View/Open |
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