Molecular Gas in nearby Early-Type Powerful Classical Radio Galaxies

Details Molecular Gas in nearby Early-Type Powerful Classical Radio Galaxies Molecular Gas in nearby Early-Type Powerful Classical Radio Galaxies

2002-11-13

arxiv.org/abs/astro-ph/0211279v1

Astronomy and Astrophysics

Astrophysics

2 pages, to appear in Active Galactic Nuclei: from Central Engine to Host Galaxy Abstract Book, meeting held in Meudon, France

Scientific paper

We report a survey for molecular gas in nearby powerful radio galaxies. Eight of the eighteen radio galaxies observed were detected with molecular masses in the range 10^7--10^9 Msun, similar to the same survey we performed towards 3C radio galaxies. The upper limits of molecular gas in the remainder are typically of 10^8 Msun, indicating that very few radiogalaxies have molecular gas reservoir with more than 10^9 Msun.

Affiliated with

Also associated with

No associations

Rating

Molecular Gas in nearby Early-Type Powerful Classical Radio Galaxies 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 Early-Type Powerful Classical Radio Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Molecular Gas in nearby Early-Type Powerful Classical Radio Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-293504