SUBMILLIMETER CONTINUUM PROPERTIES OF COLD DUST IN THE INNER DISK AND OUTFLOWS OF M 82

Deep submillimeter (submm) continuum imaging observations of the starburst galaxy M 82 are presented at 350, 450, 750, and 850 μm wavelengths, which were undertaken with the Submillimeter Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope in Hawaii. The presented maps include a co-addition of submm data mined from the SCUBA Data Archive. The co-added data produce the deepest submm continuum maps yet of M 82, in which low-level 850 μm continuum has been detected out to 1.5 kpc, at least 10% farther in radius than any previously published submm detections of this galaxy. The overall submm morphology and spatial spectral energy distribution of M 82 have a general north-south asymmetry consistent with H α and X-ray winds, supporting the association of the extended continuum with outflows of dust grains from the disk into the halo. The new data raise interesting points about the origin and structure of the submm emission in the inner disk of M 82. In particular, SCUBA short wavelength evidence of submm continuum peaks that are asymmetrically distributed along the galactic disk suggests that the inner-disk emission is reradiation from dust concentrations along a bar (or perhaps a spiral) rather than edges of a dust torus, as is commonly assumed. Higher resolution submm interferometery data from the Smithsonian Submillimeter Array and later Atacama Large Millimeter Array should spatially resolve and further constrain the reported dust emission structures in M 82.