XMM-Newton Proposal 02057401

Details XMM-Newton Proposal 02057401 XMM-Newton Proposal 02057401

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..300k&link_type=abstract

XMM-Newton Proposal ID #02057401

Statistics

N44, Xmm-Newton Proposal 02057401

Scientific paper

Super bubbles (SBs) are the complex of multiple SN explosions and strong stellar winds, hence would be a key cite of high energy activity such as high temperature plasma and particle acceleration. However, no observational evidence for particle acceleration and/or limited information of high temperature plasma has only been obtained due to the limited energy band and a poor statistics of previous observations. The X-ray brightest SB in the LMC, N44, is the best target to open new windows since a hint of cavity re-heating as well as the hard X-ray emission can be seen by ASCA and ROSAT. We thus propose a observation on N44 with XMM.

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