EG J 1809 − 2328 Mallory

نویسنده

  • Crystal L. Brogan
چکیده

We report the discovery of a partial ∼ 2 diameter non-thermal radio shell coincident with Taz, the pulsar wind nebula (PWN) in the error box of the apparently variable γ-ray source 3EG J1809−2328. We propose that this radio shell is a newly identified supernova remnant (SNR G7.5−1.7) associated with the PWN. The SNR surrounds an amorphous region of thermal X-rays detected in archival ROSAT and ASCA observations putting this system in the mixed-morphology class of supernova remnants. G7.5−1.7 is the fifth such supernova remnant coincident with a bright GeV source, and the fourth containing a pulsar wind nebulae. Subject headings: gamma rays: observations — supernova remnants — pulsars: individual(Taz) — radio continuum: ISM — X-rays: ISM — ISM: individual(G7.5−1.7)

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تاریخ انتشار 2008