The Uniformity of the Local Hot Bubble and A Pervasive Hot Medium

Details The Uniformity of the Local Hot Bubble and A Pervasive Hot Medium The Uniformity of the Local Hot Bubble and A Pervasive Hot Medium

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..108k&link_type=abstract

XMM-Newton Proposal ID #05536503

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Lhb-21, Lhb-22, Lhb-23, Xmm-Newton Proposal Id #05536503

Scientific paper

Models of the Local Hot Bubble (LHB) assume a uniform temperature and density. ROSAT, and limited XMM, and Suzaku observations suggest this is not the case, but the source of the non-uniformity is unknown. We have shown that one can use XMM spectra to isolate the emission due to the LHB without using a nearby absorbing cloud. We propose to measure the non-uniformity of the LHB, thus providing insights into the nature and origin of the LHB, the issue of Solar Wind Charge Exchange (SWCX) contribution to the LHB emission, and the nature of the diffuse emission external to the LHB.

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