Mid-IR FORCAST/SOFIA Observations of M82

Gull, G. E.; Schoenwald, J.; Morris, M. R.; Stacey, G.; Vacca, W. D.; Herter, T. L.; Tielens, A.; Nikola, T.; Adams, J. D.; Keller, L. D.; Henderson, C. P.; De Buizer, J. M.

United States, Netherlands

Abstract

We present 75'' × 75'' size maps of M82 at 6.4 μm, 6.6 μm, 7.7 μm, 31.5 μm, and 37.1 μm with a resolution of ~4'' that we have obtained with the mid-IR camera FORCAST on SOFIA. We find strong emission from the inner 60'' (~1 kpc) along the major axis, with the main peak 5'' west-southwest of the nucleus and a secondary peak 4'' east-northeast of the nucleus. The detailed morphology of the emission differs among the bands, which is likely due to different dust components dominating the continuum emission at short mid-IR wavelengths and long mid-IR wavelengths. We include Spitzer-IRS and Herschel/PACS 70 μm data to fit spectral energy distribution templates at both emission peaks. The best-fitting templates have extinctions of AV = 18 and AV = 9 toward the main and secondary emission peak and we estimated a color temperature of 68 K at both peaks from the 31 μm and 37 μm measurement. At the emission peaks the estimated dust masses are on the order of 104 M .

2012 The Astrophysical Journal
Herschel 6