Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...554l..29g&link_type=abstract
The Astrophysical Journal, Volume 554, Issue 1, pp. L29-L32.
Astronomy and Astrophysics
Astronomy
55
Galaxies: Dwarf, Galaxies: Individual: Ngc Number: Ngc 5253, Galaxies: Starburst, Galaxies: Star Clusters
Scientific paper
Hidden from optical view in the starburst region of the dwarf galaxy NGC 5253 lies an intense radio source with an unusual spectrum, which could be interpreted variously as nebular gas ionized by a young stellar cluster or nonthermal emission from a radio supernova or an active galactic nucleus. We have obtained 11.7 and 18.7 μm images of this region at the Keck telescope and find that it is an extremely strong mid-infrared emitter. The infrared-to-radio flux ratio rules out a supernova and is consistent with an H II region excited by a dense cluster of young stars. This ``supernebula'' provides at least 15% of the total bolometric luminosity of the galaxy. Its excitation requires 105-106 stars, giving it the total mass and size (1-2 pc diameter) of a globular cluster. However, its high obscuration, small size, and high gas density all argue that it is very young, no more than a few hundred thousand years old. This may be the youngest globular cluster yet observed.
Beck Sara C.
Gorjian Varoujan
Turner Jean L.
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