Molecular gas in nearby quasars

Details Molecular gas in nearby quasars Molecular gas in nearby quasars

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999alma.confe..11c&link_type=abstract

Science with the Atacama Large Millimeter Array (ALMA), Associated Universities, Inc., held October 6-8, 1999 at Carnegie Instit

Physics

Co(1-0), Quasars, Molecular Gas

Scientific paper

We present preliminary results of an ongoing survey of the CO(1-0) line emission in a sample of quasars observed with 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 MSun to 5 1010 MSun. 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

Affiliated with

Also associated with

No associations

Rating

Molecular gas in nearby quasars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Molecular gas in nearby quasars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Molecular gas in nearby quasars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1083186