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机译:Black hole accretion and star formation as drivers of gas excitation and chemistry in Markarian 231
Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, Netherlands;
School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, United Kingdom;
Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, NetherlandsBlue Sky Spectroscopy, Lethbridge, AB, CanadaMax-Planck-Institut für Astronomie, K?nigstuhl 17, 69117 Heidelberg, GermanyMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, GermanySpitzer Science Center, California Institute of Technology, MS 220-6, Pasadena, CA 91125, United StatesNaval Research Laboratory, Remote Sensing Division, Washington, DC 20375, United StatesDepartment of Astronomy, University of Maryland, College Park, MD 20742, United StatesDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United KingdomInfrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, United StatesHarvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, United StatesUniversidad de Alcalá Henares, Departamente de Física, Campus Universitario, 28871 Alcalá de Henares, Madrid, SpainDepartment of Physics, University of Lethbridge, 4401 University Drive, Lethbridge, AB, T1J 1B1, Canada;
Galaxies: active; Galaxies: individual: Mrk 231; Galaxies: ISM; Galaxies: nuclei; Galaxies: starburst; Infrared: galaxies;