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在NGC 5253中高效的恒星形成,可能是源于流的积累

J L Turner1, S C Beck2, D J Benford3

  • 1Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, California 90095-1547, USA.

Nature
|March 20, 2015
PubMed
概括

星系中的恒星形成是低效的,但NGC 5253中的密集,尘埃覆盖的气体云显示了50%以上的效率. 这种高速率可能是由气体膨胀所推动的,这解释了古代大质量恒星团的形成.

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