[Previous] | [Session 33] | [Next]
D. A. Moffett (Physics Dept., Furman University)
The last four fields from a single dish OH(1720 MHz) maser survey toward supernova remnants (Frail et al. 1996; Green et al. 1997) have been imaged at high spatial (6'') and spectral (0.34 km/s) resolution to search for compact maser emission. An additional remnant, G347.5-0.5, discovered after the survey, was also searched. Only one of the fields, toward SNR G332.0+0.2, was found to have compact OH(1720) maser emission; however, it lies well outside the radio shell.
The author(s) of this abstract have provided an email address for comments about the abstract: David.Moffett@furman.edu