An Introverted Starburst: Gas and SSC Formation in NGC 5253

Details An Introverted Starburst: Gas and SSC Formation in NGC 5253 An Introverted Starburst: Gas and SSC Formation in NGC 5253

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..217..208t&link_type=abstract

International Astronomical Union Symposium no. 217, held 14-17 July, 2003 in Sydney, Australia. Edited by P.-A. Duc, J. Braine

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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