JET-POWERED MOLECULAR HYDROGEN EMISSION FROM RADIO GALAXIES

JET-POWERED MOLECULAR HYDROGEN EMISSION FROM RADIO GALAXIES

H[subscript 2] pure-rotational emission lines are detected from warm (100-1500 K) molecular gas in [17 over 55] (31% of) radio galaxies at redshift z < 0.22 observed with the Spitzer IR Spectrograph. The summed H[subscript 2] 0-0 S(0)-S(3) line luminosities are L(H[subscript 2]) = 7 × 10[superscr...

Full description

Bibliographic Details
Main Authors: Ogle, Patrick M. (Author), Boulanger, Francois (Author), Guillard, Pierre (Author), Evans, Daniel A. (Contributor), Antonucci, Robert (Author), Appleton, P. N. (Author), Nesvadba, Nicole (Author), Leipski, Christian (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-02-26T21:00:13Z.
Subjects:
Article
Online Access:Get fulltext

Similar Items

Similar Items