Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-02-26
Astronomy and Astrophysics
Astrophysics
7 pages, 3 figures, to appear in The Astrophysical Journal
Scientific paper
10.1086/588419
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.
Brogan Crystal L.
Roberts Mallory S. E.
No associations
LandOfFree
Discovery of a New X-ray Filled Radio Supernova Remnant Around the Pulsar Wind Nebula in 3EG J1809-2328 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Discovery of a New X-ray Filled Radio Supernova Remnant Around the Pulsar Wind Nebula in 3EG J1809-2328, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discovery of a New X-ray Filled Radio Supernova Remnant Around the Pulsar Wind Nebula in 3EG J1809-2328 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-606711