Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3778
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dc.contributor.authorDeshpande, A. A-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-09-22T16:07:35Z-
dc.date.available2008-09-22T16:07:35Z-
dc.date.issued1986-05-
dc.identifier.citationAstronomy and Astrophysics, Vol. 160, No. 1, pp. 129 - 139en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3778-
dc.description.abstractRadio 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.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1986A%26A...160..129Den
dc.subjectH II Regionsen
dc.subjectRadio Sources (Astronomy)en
dc.subjectSupernova Remnantsen
dc.subjectDecametric Wavesen
dc.subjectGalactic Radiationen
dc.subjectNonthermal Radiationen
dc.subjectRadio Spectroscopyen
dc.titleObservations of the giant H II region complex W51 at decameter wavelengthsen
dc.typeArticleen
Appears in Collections:IIAP Publications

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