TY - JOUR AU - Rosenberg, M.J.F. AU - Van Der Werf, P.P. AU - Aalto, S. AU - Armus, L. AU - Charmandaris, V. AU - Díaz-Santos, T. AU - Evans, A.S. AU - Fischer, J. AU - Gao, Y. AU - González-Alfonso, E. AU - Greve, T.R. AU - Harris, A.I. AU - Henkel, C. AU - Israel, F.P. AU - Isaak, K.G. AU - Kramer, C. AU - Meijerink, R. AU - Naylor, D.A. AU - Sanders, D.B. AU - Smith, H.A. AU - Spaans, M. AU - Spinoglio, L. AU - Stacey, G.J. AU - Veenendaal, I. AU - Veilleux, S. AU - Walter, F. AU - Weiß, A. AU - Wiedner, M.C. AU - Van Der Wiel, M.H.D. AU - Xilouris, E.M. T1 - The herschel comprehensive (u)lirg emission survey (hercules): Co ladders, fine structure lines, and neutral gas cooling LA - eng PY - 2015/03/10/ T2 - Astrophysical Journal SN - 1538-4357 VL - 801 IS - 2 PB - Institute of Physics Publishing AB - (Ultra) luminous infrared galaxies ((U)LIRGs) are objects characterized by their extreme infrared (8-1000 μm) luminosities (L?LIRG > 1011 L? and L?ULIRG > 1012 L?). The Herschel Comprehensive ULIRG Emission Survey (PI: van der Werf) presents a representative flux-limited sample of 29 (U)LIRGs that spans the full luminosity range of these objects (1011 L? ≤ L?IR ≤ 1013 L?). With the Herschel Space Observatory, we observe [C II] 157 μm, [O I] 63 μm, and [O I] 145 μm line emission with Photodetector Array Camera and Spectrometer, CO J = 4-3 through J = 13-12, [C I] 370 μm, and [C I] 609 μm with SPIRE, and low-J CO transitions with ground-based telescopes. The CO ladders of the sample are separated into three classes based on their excitation level. In 13 of the galaxies, the [O I] 63 μm emission line is self absorbed. Comparing the CO excitation to the InfraRed Astronomical Satellite 60/100 μm ratio and to far infrared luminosity, we find that the CO excitation is more correlated to the far infrared colors. We present cooling budgets for the galaxies and find fine-structure line flux deficits in the [C II], [Si II], [O I], and [C I] lines in the objects with the highest far IR fluxes, but do not observe this for CO 4 ≤ J upp ≤ 13. In order to study the heating of the molecular gas, we present a combination of three diagnostic quantities to help determine the dominant heating source. Using the CO excitation, the CO J = 1-0 linewidth, and the active galactic nucleus (AGN) contribution, we conclude that galaxies with large CO linewidths always have high-excitation CO ladders, and often low AGN contributions, suggesting that mechanical heating is important. DO - 10.1088/0004-637X/801/2/72 UR - https://portalcientifico.uah.es/documentos/61578fe2d3e35f5001a23c5e DP - Dialnet - Portal de la Investigación ER -