… We must re-examine the conclusions of Braun, Goss & Lyne (1989). … The large value of n
for W28 is expected, as it is known to be expanding into a dense molecular cloud (Frail, Goss …

The satellite line of the hydroxyl radical (OH) at 1720.5 MHz has been searched for in the
direction of 66 supernova remnants in our Galaxy with the Green Bank 43-m and Parkes 64-m …

We present VLA observations in the hydroxyl line OH(1720 MHz) towards the supernova
remnant W28. These high resolution images show a more extensive distribution of 1720 MHz …

We present radio observations of a region in the vicinity of the young pulsar PSR B1853+
01 in the supernova remnant W44. The pulsar is located at the apex of an extended feature …

… The –rst Goss (1968). evidence that this may be the case was presented by Frail, Goss, & …
are seen in our data, Frail (1994b) but we fail to detect some of their weaker masers (\100 mJy)…

… DA FRAIL AND WM GosS … We first detected the OH(1720 MHz) line at several pointings
toward this SNR in Frail et at. (1996). Follow-up interferometer observations established�…

We present deep images of a region around the Crab Nebula made with the VLA, utilizing
new imaging and deconvolution algorithms in a search for a faint radio shell. The existence of …

We present the results of VLA observations in the ground-state hydroxyl (OH) transition at
1720 MHz toward 20 supernova remnants (SNRs). We detect compact emission from four …

Radio observations of the Sgr A region have been carried out at the 1720 MHz transition of
the OH molecule, using the Very Large Array and the Australia Telescope Compact Array. …

We have observed the OH (1720 MHz) line in five galactic SNRs with the VLA to measure
their magnetic field strengths using the Zeeman effect. We detected all 12 of the bright (S ν> …