to 5 1010 M. In
one of the sources, PKS2349-014, we have detected the millimeter
counterparts of
the radio lobes seen at 21 cm.
Fabienne Casoli
DEMIRM, Observatoire de Paris
Laurent Loinard
IRAM
We present preliminary results of an ongoing survey of the CO(1-0) line
emission
in
a sample of quasars observedwith the Plateau de Bure interferometer. The
sample
is extracted from a recent survey with the HST
of nearby (z < 0.3) bright quasars (Bahcall et al. 1997). First results
indicate
that a large fraction of these quasars host considerable amounts of
molecular gas (ranging from several 109 M
to 5 1010 M. In
one of the sources, PKS2349-014, we have detected the millimeter
counterparts of
the radio lobes seen at 21 cm.
Bahcall, J. N., Kirhakos, S., Schneider, D. P., 1997, ApJ 479, 642