Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-29T18:42:23.876Z Has data issue: false hasContentIssue false
  • English
  • Français

A High Resolution Optical Summary of the Structure and Dynamics of 30 Doradus

Published online by Cambridge University Press:  25 May 2016

P. Scowen ,
Y.-H. Chu  and
R. Gruendl
P. Scowen
Affiliation:
Arizona State University, Physics & Astronomy, P.O. Box 871504, Tempe, AZ 85287-1504, USA
Y.-H. Chu
Affiliation:
Dept. of Astronomy, University of Illinois, Urbana, IL 61801, USA
R. Gruendl
Affiliation:
Dept. of Astronomy, University of Illinois, Urbana, IL 61801, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present the first comparison between high resolution echelle velocity fields and a mosaic of all Hubble Space Telescope narrowband observations of 30 Doradus.

Type
Part 3. Massive Stars and 30 Doradus
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 249 - 250
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Chu, Y.-H., et al. 1996, BAAS, 188, 61.04 Google Scholar
Hunter, D.A., et al. 1995, ApJ, 448, 179 CrossRefGoogle Scholar
Scowen, P.A., et al. 1998, AJ, 116, 163 CrossRefGoogle Scholar