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- W3101107667 abstract "We report the discovery of a partial ~2deg. diameter non-thermal radio shell coincident with Taz, the pulsar wind nebula (PWN) in the error box of the apparently variable gamma-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." @default.
- W3101107667 created "2020-11-23" @default.
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- W3101107667 date "2008-07-01" @default.
- W3101107667 modified "2023-09-26" @default.
- W3101107667 title "Discovery of a New X‐Ray Filled Radio Supernova Remnant around the Pulsar Wind Nebula in 3EG J1809−2328" @default.
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- W3101107667 doi "https://doi.org/10.1086/588419" @default.
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