Searching for the engine powering the TeV source MGRO J2019+37

Details Searching for the engine powering the TeV source MGRO J2019+37 Searching for the engine powering the TeV source MGRO J2019+37

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop...79p&link_type=abstract

XMM-Newton Proposal ID #05523501

Mathematics

Logic

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Mgro J2019+37, Xmm-Newton Proposal Id #05523501

Scientific paper

The MILAGRO Collaboration has recently reported the discovery of a new extended and unidentified TeV source in the Cygnus region, MGRO J2019+37. Its location is consistent with two EGRET sources, suggesting that it could be formed by multiple unresolved sources. To find possible counterparts, we have conducted a deep radio survey discovering two jet-like sources which are positionally coincident with each of the EGRET sources and with the inner box of MGRO J2019+37. One of them has morphological and spectral characteristics similar to the microquasar 1E 1740.7-2942, the Great Annihilator at the Galactic Center. We propose to carry out a deep XMM-Newton observation covering the two radio jet sources to find their keV counterparts and constrain the mechanism responsible for the TeV emission.

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