Radio Study of a Superwind-galaxy: NGC1482

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