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Search: WFRF:(Nakanishi Kouichiro) > Mangum J. G. > Kaneko Hiroyuki > Volume Density Stru...

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Volume Density Structure of the Central Molecular Zone NGC 253 through ALCHEMI Excitation Analysis

Tanaka, Kunihiko (author)
Keio University
Mangum, J. G. (author)
National Radio Astronomy Observatory
Viti, Serena (author)
Universiteit Leiden (UL),Leiden University (UL),University College London (UCL)
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Martin, S. (author)
European Southern Observatory Santiago,Atacama Large Millimeter-submillimeter Array (ALMA)
Harada, N. (author)
The Graduate University for Advanced Studies (SOKENDAI),Academia Sinica Taiwan,National Astronomical Observatory of Japan
Sakamoto, Kazushi (author)
Academia Sinica Taiwan
Muller, Sebastien, 1976 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Yoshimura, Y. (author)
University of Tokyo, Japan
Nakanishi, Kouichiro (author)
National Astronomical Observatory of Japan,The Graduate University for Advanced Studies (SOKENDAI)
Herrero-Illana, R. (author)
Institut de Ciències de l'Espai (ICE) - CSIC,Institute of Space Sciences (ICE) - CSIC,European Southern Observatory Santiago
Emig, K.L. (author)
National Radio Astronomy Observatory
Muhle, S. (author)
Universität Bonn,University of Bonn
Kaneko, Hiroyuki (author)
Joetsu University of Education,Niigata University
Tosaki, T. (author)
Joetsu University of Education
Behrens, E. (author)
University of Virginia
Rivilla, Víctor M. (author)
Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory,Centro de Astrobiologia (CAB)
Colzi, L. (author)
Centro de Astrobiologia (CAB)
Nishimura, Y. (author)
University of Tokyo, Japan,National Astronomical Observatory of Japan
Humire, Pedro (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Bouvier, M. (author)
Universiteit Leiden (UL),Leiden University (UL)
Huang, K. Y. (author)
Universiteit Leiden (UL),Leiden University (UL)
Butterworth, Joshua (author)
Universiteit Leiden (UL),Leiden University (UL)
Meier, David S. (author)
National Radio Astronomy Observatory Socorro,New Mexico Institute of Mining and Technology
van der Werf, Paul P. (author)
Universiteit Leiden (UL),Leiden University (UL)
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 (creator_code:org_t)
2024
2024
English.
In: Astrophysical Journal. - 1538-4357 .- 0004-637X. ; 961:1
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We present a spatially resolved excitation analysis for the central molecular zone (CMZ) of the starburst galaxy NGC 253 using the data from the Atacama Large Millimeter/submillimeter Array Comprehensive High-resolution Extragalactic Molecular Inventory, whereby we explore parameters distinguishing NGC 253 from the quiescent Milky Way’s Galactic center (GC). Non-LTE analyses employing a hierarchical Bayesian framework are applied to Band 3-7 transitions from nine molecular species to delineate the position-position-velocity distributions of column density ( N H 2 ), volume density ( n H 2 ), and temperature (T kin) at 27 pc resolution. Two distinct components are detected: a low-density component with ( n H 2 , T kin ) ∼ ( 10 3.3 cm − 3 , 85 K ) and a high-density component with ( n H 2 , T kin ) ∼ ( 10 4.4 cm − 3 , 110 K ) , separated at n H 2 ∼ 10 3.8 cm − 3 . NGC 253 has ∼10 times the high-density gas mass and ∼3 times the dense-gas mass fraction of the GC. These properties are consistent with their HCN/CO ratio but cannot alone explain the factor of ∼30 difference in their star formation efficiencies (SFEs), contradicting the dense-gas mass to star formation rate scaling law. The n H 2 histogram toward NGC 253 exhibits a shallow declining slope up to n H 2 ∼ 10 6 cm − 3 , while that of the GC steeply drops in n H 2 ≳ 10 4.5 cm − 3 and vanishes at 105 cm−3. Their dense-gas mass fraction ratio becomes consistent with their SFEs when the threshold n H 2 for the dense gas is taken at ∼104.2−4.6 cm−3. The rich abundance of gas above this density range in the NGC 253 CMZ, or its scarcity in the GC, is likely to be the critical difference characterizing the contrasting star formation in the centers of the two galaxies.

Subject headings

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Meteorologi och atmosfärforskning (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Meteorology and Atmospheric Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

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