Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-29T19:25:51.133Z Has data issue: false hasContentIssue false

The New 30 Doradus

Published online by Cambridge University Press:  25 May 2016

Nolan R. Walborn
Affiliation:
STScI, 3700 San Martin Dr., Baltimore, MD 21218, USA
Rodolfo H. Barbá
Affiliation:
STScI, 3700 San Martin Dr., Baltimore, MD 21218, 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.

Recent optical and infrared studies of 30 Doradus have revealed a more complex and diverse star-formation history than previously recognized. Five spatially and/or temporally distinct populations have been identified, including a new generation currently being triggered by the R136 cluster in its surroundings. HST/NICMOS observations of the latter provide insights into the phenomena of triggered massive-star formation, as well as the global structure and evolution of the starburst region.

Type
Part 3. Massive Stars and 30 Doradus
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Rubio, M., Barbá, R.H., Walborn, N.R., Probst, R.G., Garcia, J., & Roth, M.R. 1998, AJ, 116, 1708 Google Scholar
Massey, P., & Hunter, D.A. 1998, ApJ, 493, 180 Google Scholar
Scowen, P.A., et al. 1998, AJ, 116, 163 Google Scholar
Walborn, N.R., Barbá, R.H., Brandner, W., Rubio, M., Grebel, E.K., & Probst, R.G. 1999, AJ, 117, 225 CrossRefGoogle Scholar
Walborn, N.R., & Blades, J.C. 1997, ApJS, 112, 457 Google Scholar
Walborn, N.R., & Parker, J. Wm. 1992, ApJ, 399, L87 CrossRefGoogle Scholar