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Radio Study of a Superwind-galaxy: NGC1482

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dc.contributor.author Hota, A
dc.contributor.author Saikia, D. J
dc.date.accessioned 2008-06-25T06:54:42Z
dc.date.available 2008-06-25T06:54:42Z
dc.date.issued 2003
dc.identifier.citation BASI, Vol. 31, No. 3&4, pp. 425 - 426 en
dc.identifier.uri http://hdl.handle.net/2248/2500
dc.description.abstract We 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.extent 65843 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2003BASI...31..425H en
dc.subject Galaxies:active en
dc.subject Galaxies:individual:NGC1482 en
dc.subject Galaxies:nuclei en
dc.subject Radio continuum:galaxies en
dc.title Radio Study of a Superwind-galaxy: NGC1482 en
dc.type Article en

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