No detectable supernova remnant near the pulsar PSR1930+22 (33 sources).
Observations:
We have thus observed a field (FWHB=82') centered on the pulsar position
(equinox 1950.0, RA=19 30 12.5, dec=22 15 19)
WSRT was used at 610 MHz.  A full 12h sythesis was made,
1 sigma = 2.8mJy/beam.
None of the sources in Table 1 is a 4C source. No detectable point source
coincides with the pulsar.

The resultying synthesized beam dimensions are (RAxDec) 52.5x155.5".
Table 1
Name   R.A.(1950.) err  dec(1950.) err   S(mJy)
------------------------------------------------
38W1   19 26 48.8  0.4   22 38 23  15    67   28