Yet More Multi-Wavelength Studies of Galactic Unidentified EGRET Error Boxes

Details Yet More Multi-Wavelength Studies of Galactic Unidentified EGRET Error Boxes Yet More Multi-Wavelength Studies of Galactic Unidentified EGRET Error Boxes

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0507r&link_type=abstract

American Astronomical Society, HEAD meeting #9, #5.07; Bulletin of the American Astronomical Society, Vol. 38, p.348

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Scientific paper

We will present new X-ray, radio and optical observations of sources in and around Galactic unidentified EGRET gamma-ray source error boxes. XMM-Newton Observations of the Taz PWN in GeV J1809-2327 reveal the broad X-ray emission of this rapidly moving pulsar wind nebula (RPWN), while 90 cm radio imaging with the VLA combined with archival ROSAT and ASCA X-ray data reveal a new mixed morphology supernova remnant that is the probable birth SNR of Taz. We will also show large scale extended X-ray emission associated with the PWN around PSR J2021+3651, as well as Chandra and optical observations of X-ray sources in several other EGRET error boxes.

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