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An Introverted Starburst: Gas and SSC Formation in NGC 5253

Published online by Cambridge University Press:  26 May 2016

J. L. Turner  and
S. C. Beck
J. L. Turner
Affiliation:
Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095 USA
S. C. Beck
Affiliation:
Department of Physics and Astronomy, Tel Aviv University, Ramat Aviv, Israel

Abstract

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High resolution Brackett line spectroscopy with the Keck Telescope reveals relatively narrow recombination lines toward the embedded young super star cluster nebula in NGC 5253. The gas within this nebula is almost certainly gravitationally bound by the massive and compact young star cluster.

Type
Part 2. Origin
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 208 - 209
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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