The X-Ray Emission of the Nearly Primordial Blue Compact Dwarf Galaxy SBS 0335-052

Details The X-Ray Emission of the Nearly Primordial Blue Compact Dwarf Galaxy SBS 0335-052 The X-Ray Emission of the Nearly Primordial Blue Compact Dwarf Galaxy SBS 0335-052

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop...78t&link_type=abstract

Chandra Proposal ID #01600512

Computer Science

Chandra Proposal Id #01600512

Scientific paper

Embedded in a large HI primordial cloud, with a metallicity of only Z(Sun)/41 and a stellar population not older than 100 Myr, the blue compact dwarf galaxy SBS 0335-052 is one of only two known examples of nearby young dwarf galaxies. The formation of the hot gas phase is one of the most fundamental processes in the early period of galaxy formation. Thus, its study in a very metal-deficient environment and during the early evolution phase of a galaxy is crucial for understanding the X-ray properties of high redshift galaxies. We wish to study the respective contributions of point sources and diffuse emission to the X-ray luminosity, the time evolution of the X-ray properties, and check for a possible galactic wind .

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