Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2746
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dc.contributor.authorRoy, S-
dc.date.accessioned2008-07-18T07:22:12Z-
dc.date.available2008-07-18T07:22:12Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 637 - 642en
dc.identifier.urihttp://hdl.handle.net/2248/2746-
dc.description.abstractThe central region of our milky way Galaxy still eludes a comprehensive understanding. With new observations. however. we are being able to know many of the observable properties of the sources, which allow us to better understand the actual physical processes operating in the region. Here, we discuss about the present status and the new observations in the radio wavelengths to constrain the source properties in this complex region.en
dc.format.extent193386 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectGalactic Centre Environmenten
dc.subjectInterstellar Mediumen
dc.subjectGC Filamentary Structuresen
dc.subjectGalactic Longitudeen
dc.titleRadio study of the Galactic Centre Environmenten
dc.typeArticleen
Appears in Collections:BASI Publications

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