Abstract. We have detected CO(4−3) in the z = 3.8 radio galaxy 4C 41.17 with the IRAM Interferometer. The CO is in two massive (Mdyn ∼ 6 × 1010 M) systems separated by 1.′′8 (13 kpc), and by 400 km s−1 in velocity, which coincide with two different dark lanes in a deep Lyα image. One CO component coincides with the cm-radio core of the radio galaxy, and its redshift is close to that of the He λ 1640 AGN line. The second CO component is near the base of a cone-shaped region southwest of the nucleus, which resembles the emission-line cones seen in nearby AGN and starburst galaxies. The characteristics of the CO sources and their mm/submm dust continuum are similar to those found in ultraluminous IR galaxies and in some high-z radio galaxies...
Appearing in the 2004 October 10 issue of the Astrophysical Journal Letters, Volume 614, L5-L8We rep...
We report IRAM millimeter interferometry of three zsimilar to2.4-3.4 Submillimeter Common-User Bolom...
5 pages, 3 figures, LaTex (l-aa.sty, psfig.sty), also available at http://www.ast.cam.ac.uk/~rgmWe r...
We have detected CO(4-3) in the $z=3.8$ radio galaxy 4C 41.17 with the IRAM Interferometer. The CO i...
34 pages, 5 figures, accepted for publication in The Astrophysical JournalWe report the detection of...
There is reason to suspect that 4C 41.17, a radio galaxy at z = 3.8, contains a large quantity of en...
We report on the detection of the lowest CO$~J={1} {-} {0}$ transition in the powerful high-redshift...
Using the IRAM interferometer we have detected J=4-->3 and 5-- >4 CO line emission toward the radio ...
Dense molecular clouds are critical to the activity occurring in galactic nuclei. They are the activ...
The peaking of quasar density at z ∼ 2 as well as the stellar population analysis of galaxies in the...
We report a sensitive search for redshifted CO J = 3-2 emission from the weak radio galaxy 53W002 at...
We report the detection of luminous CO(3-2) line emission in the halo of the z = 2.6 radio galaxy (H...
We have used the Owens Valley Millimeter Array to conduct a sensitive search for CO (1 - 0) emission...
There is reason to suspect that 4C 41.17, a radiogalaxy at z = 3.800±0.003, contains a large quantit...
International audienceWe present CO observations of nine ultra-luminous infrared galaxies (ULIRGs) a...
Appearing in the 2004 October 10 issue of the Astrophysical Journal Letters, Volume 614, L5-L8We rep...
We report IRAM millimeter interferometry of three zsimilar to2.4-3.4 Submillimeter Common-User Bolom...
5 pages, 3 figures, LaTex (l-aa.sty, psfig.sty), also available at http://www.ast.cam.ac.uk/~rgmWe r...
We have detected CO(4-3) in the $z=3.8$ radio galaxy 4C 41.17 with the IRAM Interferometer. The CO i...
34 pages, 5 figures, accepted for publication in The Astrophysical JournalWe report the detection of...
There is reason to suspect that 4C 41.17, a radio galaxy at z = 3.8, contains a large quantity of en...
We report on the detection of the lowest CO$~J={1} {-} {0}$ transition in the powerful high-redshift...
Using the IRAM interferometer we have detected J=4-->3 and 5-- >4 CO line emission toward the radio ...
Dense molecular clouds are critical to the activity occurring in galactic nuclei. They are the activ...
The peaking of quasar density at z ∼ 2 as well as the stellar population analysis of galaxies in the...
We report a sensitive search for redshifted CO J = 3-2 emission from the weak radio galaxy 53W002 at...
We report the detection of luminous CO(3-2) line emission in the halo of the z = 2.6 radio galaxy (H...
We have used the Owens Valley Millimeter Array to conduct a sensitive search for CO (1 - 0) emission...
There is reason to suspect that 4C 41.17, a radiogalaxy at z = 3.800±0.003, contains a large quantit...
International audienceWe present CO observations of nine ultra-luminous infrared galaxies (ULIRGs) a...
Appearing in the 2004 October 10 issue of the Astrophysical Journal Letters, Volume 614, L5-L8We rep...
We report IRAM millimeter interferometry of three zsimilar to2.4-3.4 Submillimeter Common-User Bolom...
5 pages, 3 figures, LaTex (l-aa.sty, psfig.sty), also available at http://www.ast.cam.ac.uk/~rgmWe r...