Note: this is an archived version which has been superseded.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.
X-ray: Centrally concentrated, thermal spectrum, plus pulsar nebula.
Point sources: Pulsar within the boundary of the remnant.
Distance: HI absorption indicates 2.5 kpc.

References:

Last updated: 8 Nov 2001


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