Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2735
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dc.contributor.authorDeshpande, A. A-
dc.contributor.authorShevgaonkar, R. K-
dc.contributor.authorSastry, Ch. V-
dc.date.accessioned2008-07-18T05:21:17Z-
dc.date.available2008-07-18T05:21:17Z-
dc.date.issued1984-07-
dc.identifier.citationAstrophysics and Space Science, Vol. 102, No. 1, pp. 21 – 27en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/2735-
dc.description.abstractA map of Rosette Nebula in continuum absorption is made at 34.5 MHz using the Decameter Wave Radio Telescoe at Gauribidanur, India, with a resolution of 26×40, is presented. These observations are combined with the 2700 MHz measurements of Grahamet al. (1982) to derive the electron temperature distribution across the nebula. It is found that the temperatures in the southeastern parts of the nebula are around 5000 K and increase up to 8000 K towards the northwestern regions. It is suggested that the lower electron temperatures in the southeastern regions are due to the presence of more dust there compared to other regions in the nebula.en
dc.format.extent640428 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1984Ap%26SS.102...21Den
dc.relation.urihttp://www.springerlink.com/content/w6n22685l71318v7/-
dc.subjectDecametric Wavesen
dc.subjectElectron Energyen
dc.subjectHydrogen Clouds-
dc.subjectNebulae, Radio Sources (Astronomy)-
dc.subjectAbsorption Spectra-
dc.subjectAstronomical Maps-
dc.subjectContinuous Spectra-
dc.subjectRadio Telescopes-
dc.subjectRosette Shapes-
dc.titleObservations of the Rosette Nebula using the Decameter Wave Radio Telescope at Gauribidanuren
dc.typeArticleen
Appears in Collections:IIAP Publications

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