Note: this is an archived version which has been superseded. The current SNR catalogue is at http://www.mrao.cam.ac.uk/surveys/snrs/

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 2.8 kpc.

References:

Last updated: 30 May 2014


home | documentation | detailed listings | summary listings

Dave Green/Cambridge, UK/D.A.Green@mrao.cam.ac.uk