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Fire in the Heart: A Characterization of the High Kinetic Temperatures and Heating Sources in the Nucleus of NGC253

Mangum, Jeffrey G. (författare)
National Radio Astronomy Observatory
Ginsburg, Adam G. (författare)
National Radio Astronomy Observatory Socorro
Henkel, Christian (författare)
King Abdulaziz University,Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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Menten, Karl M. (författare)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Aalto, Susanne, 1964 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
van der Werf, Paul (författare)
Universiteit Leiden (UL),Leiden University (UL)
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 (creator_code:org_t)
2019-01-30
2019
Engelska.
Ingår i: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 871:2
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • The nuclear starburst within the central similar to 15 '' (similar to 250 pc; 1 '' similar or equal to 17 pc) of NGC 253 has been extensively studied as a prototype for the starburst phase in galactic evolution. Atacama Large Millimeter/submillimeter Array (ALMA) imaging within receiver Bands 6 and 7 has been used to investigate the dense gas structure, kinetic temperature, and heating processes that drive the NGC 253 starburst. A total of 29 transitions from 15 molecular species/isotopologues have been identified and imaged at 1.'' 5-0.'' 4 resolution, allowing for the identification of five of the previously studied giant molecular clouds within the central molecular zone (CMZ) of NGC 253. Ten transitions from the formaldehyde (H2CO) molecule have been used to derive the kinetic temperature within the similar to 0.'' 5-5 '' dense gas structures imaged. On similar to 5 '' scales we measure T-K greater than or similar to 50 K, while on size scales less than or similar to 1 '' we measure T-K greater than or similar to 300 K. These kinetic temperature measurements further delineate the association between potential sources of dense gas heating. We have investigated potential heating sources by comparing our measurements to models that predict the physical conditions associated with dense molecular clouds that possess a variety of heating mechanisms. This comparison has been supplemented with tracers of recently formed massive stars (Br gamma) and shocks ([Fe II]). Derived molecular column densities point to a radially decreasing abundance of molecules with sensitivity to cosmic-ray and mechanical heating within the NGC 253 CMZ. These measurements are consistent with radio spectral index calculations that suggest a higher concentration of cosmic-ray-producing supernova remnants within the central 10 pc of NGC 253.

Ämnesord

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)
NATURVETENSKAP  -- Fysik -- Annan fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Other Physics Topics (hsv//eng)

Nyckelord

galaxies: spiral
galaxies: starburst
galaxies: individual (NGC 253)
galaxies: nuclei
ISM: molecules
galaxies: active

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