A High Resolution Map of 12CO J=6-5 Emission in the Starburst Galaxy M82

Abstract

We present a map of 12CO J=6-5 emission of the nuclear region of the nearby starburst galaxy M82 at resolution 7" taken with the James Clerk Maxwell Telescope (JCMT). This is the highest resolution map yet available at this transition. A detailed quantitative comparison is made with emission at 12CO J=1-0 at the same resolution yielding new insights into the excitation of molecular gas in this galaxy. The excitation is found to be highest in the central area of the starburst region where the ratio r_61 = 12CO J=6-5/12CO J=1-0 is as high as 0.5, compared to the mean value over the starburst region of 0.24. The excitation ratio peaks along the inner edge of the molecular ring outlined by atomic and molecular gas at lower excitation, and also in two spurs extending northward from the disk toward the outflow associated with the supwerwind. Emission with higher than avarage excitation is also found to be associated with the supershell surrounding the luminous SNR candidate 41.9+58, and possibly on a larger scale in gas whose orbits are strongly influenced by the stellar bar. The higher excitation in M82 is likely to be caused predominantly by local increases in kinetic temperature and/or geometric filling factor of a pre-existing higher excitation component, and less likely to be caused by local increases in gas density.

References in corpus (7)

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• Star-formation in the central kpc of the starburst/LINER galaxy NGC1614
• Formaldehyde as a Tracer of Extragalactic Molecular Gas I. Para-H_2CO Emission From M 82
• Formaldehyde Densitometry of Starburst Galaxies: Density-Independent Global Star Formation
• A Census of the High-Density Molecular Gas in M82
• Tracing high density gas in M 82 and NGC 4038
• High-velocity-resolution observations of OH main line lasers in the M82 starburst
• Evolving Starburst Modeling of FIR/sub-mm/mm Line Emission. II. Application to M 82
• The MALATANG survey: Dense gas distribution on sub-kiloparsec scales across the disk of M82
• Extragalactic H3O+: Some Consequences