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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2500
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dc.contributor.authorHota, A-
dc.contributor.authorSaikia, D. J-
dc.date.accessioned2008-06-25T06:54:42Z-
dc.date.available2008-06-25T06:54:42Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 425 - 426en
dc.identifier.urihttp://hdl.handle.net/2248/2500-
dc.description.abstractWe present GMRT and VLA observations of the superwind galaxy, NGC1482, which has been discovered to have a remarkable hour-glass shaped optical emission line outflow on both sides of the galactic disk. The central region has a prominent compact component, and suggestions of additional compact features.en
dc.format.extent65843 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..425Hen
dc.subjectGalaxies:activeen
dc.subjectGalaxies:individual:NGC1482en
dc.subjectGalaxies:nucleien
dc.subjectRadio continuum:galaxiesen
dc.titleRadio Study of a Superwind-galaxy: NGC1482en
dc.typeArticleen
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