G34.7−0.4

W44, 3C392

Notes: Has been called G34.6−0.5.

Radio: Distorted shell, brighter to the E, with pulsar and associated nebula.
Optical: Diffuse emission.
X-ray: Centrally concentrated, thermal spectrum, plus pulsar wind nebula.
Point sources: Pulsar within the boundary of the remnant.
Distance: HI absorption indicates ~3 kpc.

References:

Last updated: 16 Jun 2017


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Dave Green/Cambridge, UK/