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Star formation and gas distribution in the Magellanic Spiral NGC 4214
V.J. McIntyre
Physics Dept, University of Wollongong
Northfields Ave, NSW 2522, Australia
vjm@davinci.sci.uow.edu.au
Abstract:
I present new high-resolution observations of the HI in NGCб 4214 made as part of a study of the small-scale kinematics and star formation regions of the galaxy.
Keywords: galaxies; individual (NGC 4214) - galaxies: kinematics and dynamics - radio lines: galaxies
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