Gas kinematics in the halo of the warm ULIRG PKS1345+12

Details Gas kinematics in the halo of the warm ULIRG PKS1345+12 Gas kinematics in the halo of the warm ULIRG PKS1345+12

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ap%26ss.324..225r&link_type=abstract

Astrophysics and Space Science, Volume 324, Issue 2-4, pp. 225-229

Astronomy and Astrophysics

Astrophysics

Radio Galaxies, Ulirgs, Kinematics

Scientific paper

We use long-slit spectra taken with the William Herschel Telescope on La Palma and high-resolution Hubble Space Telescope imaging to study the gas kinematic in the halo of the ultraluminous infrared/radio galaxy PKS1345+12 ( z=0.122). Our long-slit spectra show line splitting at the locations of massive star clusters ( 106

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