...
In the
Torrelles et al. (1992)
map, the presence of extended emission is suggested only by the weakest contours, below the
level.
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
... uncertain
The 8.4 GHz observations were conducted by
Hunter et al. (1999)
in snapshot mode, with a few minutes of integration, whereas our 8.4 GHz observations last for about one hour, allowing a significant sensitivity improvement.
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Copyright ESO 2006