Next Section: Introduction

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 NGC 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

© Copyright Astronomical Society of Australia 1997