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26 April 2024
 
  » arxiv » astro-ph/0311165

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An extragalactic supernebula confined by gravity
J. L. Turner ; S. C. Beck ; L. P. Crosthwaite ; J. E. Larkin ; I. S. McLean ; D. S. Meier ;
Date 7 Nov 2003
Journal Nature 423 (2003) 621-623
Subject astro-ph
Affiliation1,3), J. E. Larkin , I. S. McLean , and D. S. Meier (1,4) ( UCLA, Tel Aviv University, Astute Networks, University of Illinois, Urbana
AbstractLittle is known about the origins of the giant star clusters known as globular clusters. How can hundreds of thousands of stars form simultaneously in a volume only a few light years across the distance of the sun to its nearest neighbor? Radiation pressure and winds from luminous young stars should disperse the star-forming gas and disrupt the formation of the cluster. Globular clusters in our Galaxy cannot provide answers; they are billions of years old. Here we report the measurement of infrared hydrogen recombination lines from a young, forming super star cluster in the dwarf galaxy, NGC 5253. The lines arise in gas heated by a cluster of an estimated million stars, so young that it is still enshrouded in gas and dust, hidden from optical view. We verify that the cluster contains 4000-6000 massive, hot "O" stars. Our discovery that the gases within the cluster are bound by gravity may explain why these windy and luminous O stars have not yet blown away the gases to allow the cluster to emerge from its birth cocoon. Young clusters in "starbursting" galaxies in the local and distant universe may be similarly gravitationally confined and cloaked from view.
Source arXiv, astro-ph/0311165
Other source [GID 438207] pmid12789332
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