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A New Investigation of the 30 Doradus Region with the Australia Telescope Compact Array

Published online by Cambridge University Press:  25 May 2016

J. S. Lazendic ,
R. F. Haynes ,
J. R. Dickel ,
P. A. Jones ,
G. L. White  and
M. Costa
J. S. Lazendic
Affiliation:
Centre for Astronomy, University of Western Sydney, Nepean, Australia
R. F. Haynes
Affiliation:
Australia Telescope National Facility, CSIRO, Australia
J. R. Dickel
Affiliation:
Astronomy Department, University of Illinois, Urbana, IL 61801, USA
P. A. Jones
Affiliation:
Centre for Astronomy, University of Western Sydney, Nepean, Australia
G. L. White
Affiliation:
Centre for Astronomy, University of Western Sydney, Nepean, Australia
M. Costa
Affiliation:
Physics Department, University of Tasmania, Australia

Extract

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30 Doradus is a giant H II region in the Large Magellanic Cloud (Bode 1801). It is the nearest extragalactic giant H II region and the location of active star formation. The complex nature of this extended region provides an excellent opportunity to investigate the impact of massive stars on the structure of the interstellar medium. Specifically the presence of supernova remnants (SNRs) is expected to play an important role.

Type
Part 3. Massive Stars and 30 Doradus
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 251 - 253
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Bode, J. 1801, Algemeine Beschreibung und Nachweisung der Gestirne, (Berlin: Beym Verfasser)Google Scholar
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Smith, R. C. 1997, http://www.astro.lsa.umich.edu/ncels/mcsurvey.html Google Scholar