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BAT AGN Spectroscopic Survey. XX. Molecular Gas in Nearby Hard-X-Ray-selected AGN Galaxies
Koss,Michael J.1; Strittmatter,Benjamin2; Lamperti,Isabella3; Shimizu,Taro4; Trakhtenbrot,Benny5; Saintonge,Amelie3; Treister,Ezequiel6; Cicone,Claudia7; Mushotzky,Richard8; Oh,Kyuseok9,10; Ricci,Claudio11,12,13; Stern,Daniel14; Ananna,Tonima Tasnim15; Bauer,Franz E.16,17,18; Privon,George C.19; B?r,Rudolf E.2; Breuck,Carlos De20; Harrison,Fiona21; Ichikawa,Kohei22; Powell,Meredith C.23; Rosario,David24; Sanders,David B.25; Schawinski,Kevin26; Shao,Li27; Megan Urry,C.28; Veilleux,Sylvain8
2021-02-01
Source PublicationThe Astrophysical Journal Supplement Series
ISSN0067-0049
Volume252Issue:2
AbstractAbstract We present the host-galaxy molecular gas properties of a sample of 213 nearby (0.01??1044 erg s?1 ) increases by ~10–100 between a molecular gas mass of 108.7M⊙ and 1010.2M⊙. AGN galaxies with a higher Eddington ratio (log(L/LEdd) > ?1.3) tend to have higher molecular gas masses and gas fractions. The log(NH/ cm?2 ) > 23.4) of AGN galaxies with higher column densities are associated with lower depletion timescales and may prefer hosts with more gas centrally concentrated in the bulge that may be more prone to quenching than galaxy-wide molecular gas. The significant average link of host-galaxy molecular gas supply to supermassive black hole (SMBH) growth may naturally lead to the general correlations found between SMBHs and their host galaxies, such as the correlations between SMBH mass and bulge properties, and the redshift evolution of star formation and SMBH growth.
KeywordActive galactic nuclei AGN host galaxies Molecular gas Surveys X-ray active galactic nuclei Survival analysis Submillimeter astronomy High energy astrophysics Seyfert galaxies Catalogs
DOI10.3847/1538-4365/abcbfe
Language英语
WOS IDIOP:0067-0049-252-2-abcbfe
PublisherThe American Astronomical Society
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/60672
Collection中国科学院国家天文台
Corresponding AuthorKoss,Michael J.
Affiliation1.Eureka Scientific, 2452 Delmer Street, Suite 100, Oakland, CA 94602-3017, USA; mike.koss@eurekasci.com
2.Institute for Particle Physics and Astrophysics, ETH Zürich, Wolfgang-Pauli-Strasse 27, CH-8093 Zürich, Switzerland
3.Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
4.Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany
5.School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel
6.Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile
7.Institute of Theoretical Astrophysics, University of Oslo, Postboks 1029, Blindern No-0315 Oslo, Norway
8.Department of Astronomy, University of Maryland, College Park, MD 20742, USA
9.Korea Astronomy & Space Science institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea
10.Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502, Japan
11.Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago 22, Chile
12.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China
13.George Mason University, Department of Physics & Astronomy, MS 3F3, 4400 University Drive, Fairfax, VA 22030, USA
14.Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, MS 169-224, Pasadena, CA 91109, USA
15.Department of Physics & Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755, USA
16.Instituto de Astrofísica and Centro de Astroingeniería, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile
17.Millennium Institute of Astrophysics (MAS), Nuncio Monse?or Sótero Sanz 100, Providencia, Santiago, Chile
18.Space Science Institute, 4750 Walnut Street, Suite 205, Boulder, CO 80301, USA
19.Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611, USA
20.European Southern Observatory, Karl Schwarzschild Str 2, D-85748 Garching, Germany
21.Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA
22.Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai 980-8578, Japan
23.Institute of Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA
24.Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, DH1 3LE Durham, UK
25.Institute for Astronomy, 2680 Woodlawn Drive, University of Hawaii, Honolulu, HI 96822, USA
26.Modulos AG, Technoparkstrasse 1, CH-8005 Zurich, Switzerland
27.National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China
28.Yale Center for Astronomy & Astrophysics, Physics Department, New Haven, CT 06520, USA
Recommended Citation
GB/T 7714
Koss,Michael J.,Strittmatter,Benjamin,Lamperti,Isabella,et al. BAT AGN Spectroscopic Survey. XX. Molecular Gas in Nearby Hard-X-Ray-selected AGN Galaxies[J]. The Astrophysical Journal Supplement Series,2021,252(2).
APA Koss,Michael J..,Strittmatter,Benjamin.,Lamperti,Isabella.,Shimizu,Taro.,Trakhtenbrot,Benny.,...&Veilleux,Sylvain.(2021).BAT AGN Spectroscopic Survey. XX. Molecular Gas in Nearby Hard-X-Ray-selected AGN Galaxies.The Astrophysical Journal Supplement Series,252(2).
MLA Koss,Michael J.,et al."BAT AGN Spectroscopic Survey. XX. Molecular Gas in Nearby Hard-X-Ray-selected AGN Galaxies".The Astrophysical Journal Supplement Series 252.2(2021).
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