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26 April 2024
 
  » arxiv » 1005.1877

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Probing the molecular interstellar medium of M82 with Herschel-SPIRE spectroscopy
P. Panuzzo ; N. Rangwala ; A. Rykala ; K. G. Isaak ; J. Glenn ; C. D. Wilson ; R. Auld ; M. Baes ; M. J. Barlow ; G. J. Bendo ; J. J. Bock ; A. Boselli ; M. Bradford ; V. Buat ; N. Castro-Rodríguez ; P. Chanial ; S. Charlot ; L. Ciesla ; D. L. Clements ; A. Cooray ; D. Cormier ; L. Cortese ; J. I. Davies ; E. Dwek ; S. A. Eales ; D. Elbaz ; T. Fulton ; M. Galametz ; F. Galliano ; W. K. Gear ; H. L. Gomez ; M. Griffin ; S. Hony ; L. R. Levenson ; N. Lu ; S. Madden ; B. O'Halloran ; K. Okumura ; S. Oliver ; M. J. Page ; A. Papageorgiou ; T. J. Parkin ; I. Pérez-Fournon ; M. Pohlen ; E. T. Polehampton ; E. E. Rigby ; H. Roussel ; N. Sacchi ; M. Sauvage ; B. Schulz ; M. R. P. Schirm ; M. W. L. Smith ; L. Spinoglio ; J. A. Stevens ; S. Srinivasan ; M. Symeonidis ; B. Swinyard ; M. Trichas ; M. Vaccari ; L. Vigroux ; H. Wozniak ; G. S. Wright ; W. W. Zeilinger ;
Date 11 May 2010
AbstractWe present the observations of the starburst galaxy M82 taken with the Herschel SPIRE Fourier Transform Spectrometer. The spectrum (194-671 {mu}m) shows a prominent CO rotational ladder from J = 4-3 to 13-12 emitted by the central region of M82. The fundamental properties of the gas are well constrained by the high J lines observed for the first time. Radiative transfer modeling of these high-S/N 12CO and 13CO lines strongly indicates a very warm molecular gas component at ~500 K and pressure of ~3x10^6 K cm^-3, in good agreement with the H_2 rotational lines measurements from Spitzer and ISO. We suggest that this warm gas is heated by dissipation of turbulence in the interstellar medium (ISM) rather than X-rays or UV flux from the straburst. This paper illustrates the promise of the SPIRE FTS for the study of the ISM of nearby galaxies.
Source arXiv, 1005.1877
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