Investigating the nature of the candidate SNR G29.37+0.10

Details Investigating the nature of the candidate SNR G29.37+0.10 Investigating the nature of the candidate SNR G29.37+0.10

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cxo..prop.2833t&link_type=abstract

Chandra proposal ID #11500541

Computer Science

Scientific paper

The new supernova remnant (SNR) candidate G29.37+0.10 is a very peculiar object: a bright jet or filament-like structure lying at the centre of a faint radio shell. The nature of the jet structure is unclear. Originally interpreted as a radio Galaxy, the association with a shell SNR is also suggesting a pulsar wind nebula (PWN) or microquasar system. Two X-ray point sources and a hint of diffuse emission are detected on the edge of the northeastern radio lobe in archival data, one of them being variable. Recently HESS has discovered a large complex of TeV emission, HESS J1843-033, the north eastern wing of which is coincident with G29.37+0.10. We propose a deep Chandra observation to determine the origin of the high energy particles and the actual nature of this unusual SNR candidate.

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