The following document lists the file abstract/PBARTHEL_PDB_BLRG.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
Broad line radio galaxies (BLRGs) display properties in between those of radio-loud quasars and narrow line radio galaxies. IRAS far-infrared energy distributions of some BLRGs indicate the presence of a hot dust component, whereas optical spectra of several BLRGs have revealed an unusually bright starlight component. We wish to use ISOPHOT to observe a sample of broad line radio galaxies in order to examine this trend further. The resulting data will be used to investigate (circum)nuclear star formation in BLRGs and to address the place of the BLRG class in unified schemes for radio-loud objects.