The following document lists the file abstract/GKRISHNA_BRGALA_2.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
We request for a total 2 hours time: (i) To carry out a critical follow-up of the two brightest and specially interesting members of our sample of intrinsically weak radio galaxies covered in our ISO imaging project.The proposed observations, prompted by the just reduced ISO data, consist of a CVF spectroscopic search for PAH features, which would provide crucial evidence on the current controversy about nature of central engines of weak radio galaxies being basically different from those of powerful radio galaxies. We also propose 60 micron photometry of these two bright galaxies. (ii) To complete ISOCAM imaging of our 6 most promising target galaxies out of those which have not yet been scheduled since they were originally assigned Grade 3 simply because of falling outside the ISO range within its originally expected lifetime.