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Observations of the Rosette Nebula using the Decameter Wave Radio Telescope at Gauribidanur

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dc.contributor.author Deshpande, A. A
dc.contributor.author Shevgaonkar, R. K
dc.contributor.author Sastry, Ch. V
dc.date.accessioned 2008-07-18T05:21:17Z
dc.date.available 2008-07-18T05:21:17Z
dc.date.issued 1984-07
dc.identifier.citation Astrophysics and Space Science, Vol. 102, No. 1, pp. 21 – 27 en
dc.identifier.issn 0004-640X
dc.identifier.uri http://hdl.handle.net/2248/2735
dc.description.abstract A 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.extent 640428 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher D. Reidel Publishing Co. en
dc.relation.uri http://adsabs.harvard.edu/abs/1984Ap%26SS.102...21D en
dc.relation.uri http://www.springerlink.com/content/w6n22685l71318v7/
dc.subject Decametric Waves en
dc.subject Electron Energy en
dc.subject Hydrogen Clouds
dc.subject Nebulae, Radio Sources (Astronomy)
dc.subject Absorption Spectra
dc.subject Astronomical Maps
dc.subject Continuous Spectra
dc.subject Radio Telescopes
dc.subject Rosette Shapes
dc.title Observations of the Rosette Nebula using the Decameter Wave Radio Telescope at Gauribidanur en
dc.type Article en


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