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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1556
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dc.contributor.authorDeshpande, A.A.-
dc.contributor.authorShevgaonkar, R.K.-
dc.contributor.authorSastry, Ch.V.-
dc.date.accessioned2006-12-05T10:38:34Z-
dc.date.available2006-12-05T10:38:34Z-
dc.date.issued1984-07-
dc.identifier.citationAstrophysics and Space Science, 1984, Vol.102, p21-27en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2289/1556-
dc.descriptionScanned article available at the NASA Astrophysics Data System (Alternative location)-
dc.description.abstractA map of Rosette Nebula in continuum absorption, made at 34.5 MHz using the Decameter Wave Radio Telescope at Gauribidanur, India, with a resolution of 26 min x 40 min, is presented. These observations are combined with the 2700 MHz measurements of Graham et 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.extent592496 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1984Ap&SS.102...21Den
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984Ap%26SS.102...21D&link_type=ARTICLE&db_key=ASTen
dc.rights(1984) Kluwer Academic Publishers.en
dc.subjectDECAMETRIC WAVES,en
dc.subjectELECTRON ENERGYen
dc.subjectHYDROGEN CLOUDS,en
dc.subjectNEBULAE,en
dc.subjectRADIO SOURCES (ASTRONOMY),en
dc.subjectABSORPTION SPECTRA,en
dc.subjectASTRONOMICAL MAPS,en
dc.subjectCONTINUOUS SPECTRA,en
dc.subjectRADIO TELESCOPES,en
dc.subjectROSETTE SHAPESen
dc.titleObservations of the Rosette Nebula using the decameter wave radio telescope at Gauribidanur.en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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