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2005MNRAS.356..998H - Mon. Not. R. Astron. Soc., 356, 998-1008 (2005/January-3)
A radio study of the superwind galaxy NGC 1482.
HOTA A. and SAIKIA D.J.
Abstract (from CDS):
The HI observations with the GMRT show two blobs of emission on opposite sides of the central region. These are rotating about the centre of the galaxy and are located at ∼2.4 kpc from it. In addition, these observations also reveal a multicomponent HI absorption profile against the central region of the radio source, with a total width of ∼250 km/s. The extreme blue- and redshifted absorption components are at 1688 and 1942 km/s, respectively, while the peak absorption is at 1836 km/s. This is consistent with the heliocentric systemic velocity of 1850±20 km/s, estimated from a variety of observations. We discuss possible implications of these results.
Abstract Copyright: 2004 RAS
Journal keyword(s): galaxies: active - galaxies: individual: NGC 1482 - galaxies: kinematics and dynamics - galaxies: starburst - radio continuum: galaxies - radio lines: galaxies
Nomenclature: Table 4: [HS2005] JHHMMSS.ss+DDMMSS.s N=7.
Simbad objects: 23