The Nearby Low Metallicity Starburst NGC~346: a High Redshift Starburst Analogue

Details The Nearby Low Metallicity Starburst NGC~346: a High Redshift Starburst Analogue The Nearby Low Metallicity Starburst NGC~346: a High Redshift Starburst Analogue

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..553c&link_type=abstract

Chandra Proposal ID #02200383

Physics

Chandra Proposal Id #02200383

Scientific paper

Hot stars form in groups in spiral and irregular galaxies. Understanding the X-ray emission from starburst regions depends on disentangling point source from diffuse emission. We request a 100 ksec ACIS-I observation of an important nearby "starburst analogue", NGC 346 in the LMC. This observation will allow us to study the extended emission, the emission from evolved O stars, and to look for candidate collapsed objects and proto-stars in this low-metallicity stellar group.

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