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HST/NICMOS Survey in the 30 Doradus Nebular Filaments

Published online by Cambridge University Press:  25 May 2016

Rodolfo H. Barbá ,
Nolan R. Walborn ,
Wolfgang Brandner ,
Ronald G. Probst ,
Mónica Rubio  and
Eva K. Grebel
Rodolfo H. Barbá
Affiliation:
STScI, 3700 San Martin Dr., Baltimore, MD 21218, USA
Nolan R. Walborn
Affiliation:
STScI, 3700 San Martin Dr., Baltimore, MD 21218, USA
Wolfgang Brandner
Affiliation:
IPAC, Caltech, 770 South Wilson Ave., Pasadena, CA 91125, USA
Ronald G. Probst
Affiliation:
CTIO, NOAO, Casilla 603, La Serena, Chile
Mónica Rubio
Affiliation:
Depto. de Astronomía, Univ. de Chile, Casilla 36-D, Santiago, Chile
Eva K. Grebel
Affiliation:
Lick Observatory, Univ. of California, Santa Cruz, CA 95064, USA

Abstract

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On the basis of ample evidence accumulated during recent years for current star formation within the 30 Doradus Nebula, which appears to have been triggered by the massive central cluster (R136) in and just beyond the curved nebular filaments surrounding it, an HST/NICMOS survey of these regions was undertaken.

Type
Part 3. Massive Stars and 30 Doradus
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 245 - 246
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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