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Star Formation and Gas Distribution in the Magellanic Spiral NGC 4214

Published online by Cambridge University Press:  05 March 2013

V. J. McIntyre
V. J. McIntyre*
Affiliation:
Physics Department, University of Wollongong, Northfields Ave, Wollongong, NSW 2522, Australia. vjm@davinci.sci.uow.edu.au
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Abstract

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I present new high-resolution observations of the HI in NGC 4214 made as part of a study of the small-scale kinematics and star formation regions of the galaxy.

Type
Hi in the Local Universe
Information
Publications of the Astronomical Society of Australia , Volume 14 , Issue 1 , 1997 , pp. 122 - 123
Copyright
Copyright © Astronomical Society of Australia 1997

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