XMM-Newton Proposal 02026501

Details XMM-Newton Proposal 02026501 XMM-Newton Proposal 02026501

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..140p&link_type=abstract

XMM-Newton Proposal ID #02026501

Computer Science

He 2-10, Xmm-Newton Proposal 02026501

Scientific paper

The blue compact dwarf (BCD) galaxy He 2-10 is an excellent nearby laboratory to study the formation and evolution of hot plasma in the presence of ongoing and intense starburst activity. Previous multiwavelength studies have revealed that the energetic output of the starburst has led to a bipolar outflow of hot gas expanding from the nuclear starburst region into the ambient HI halo with a velocity of ~250 km/sec. Deep XMM-Newton X-ray data will allow us to study the metallicity and thermodynamic properties of the extended X-ray emission in He 2-10 and put constraints on its starburst-driven evolution.

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