The composite unidentified source HESS J1843-033

Details The composite unidentified source HESS J1843-033 The composite unidentified source HESS J1843-033

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop..168t&link_type=abstract

XMM-Newton Proposal ID #06549601

Mathematics

Logic

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Hess J1843-033

Scientific paper

In a survey of the Galactic plane performed in 2007 with the High Energy Stereoscopic System (H.E.S.S.) many new sources have been discovered and most of them are still unidentified. We propose to use XMM-Newton to perform follow-up observations on one of the brightest newly discovered sources, HESS J1843-033, to identify its possible X-ray counterparts. An offset PWN is one of the possible explanations for HESS J1843-033, but this hypothesis is still under investigation. The aim is to obtain the morphological and spectral information of the possible counterparts in helping to understand the emission mechanism of this source.

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