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MID-IR FORCAST/SOFIA OBSERVATIONS OF M82

Journal Article · · Astrophysical Journal Letters
; ; ; ; ; ;  [1]; ;  [2];  [3];  [4];  [5]
  1. Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States)
  2. Universities Space Research Association, NASA Ames Research Center, MS 211-3, Moffett Field, CA 94035 (United States)
  3. Department of Physics, Ithaca College, Ithaca, NY 14850 (United States)
  4. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547 (United States)
  5. Leiden Observatory, P.O. Box 9513, Leiden, 2300 RA (Netherlands)
We present 75'' Multiplication-Sign 75'' size maps of M82 at 6.4 {mu}m, 6.6 {mu}m, 7.7 {mu}m, 31.5 {mu}m, and 37.1 {mu}m with a resolution of {approx}4'' that we have obtained with the mid-IR camera FORCAST on SOFIA. We find strong emission from the inner 60'' ({approx}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 {mu}m data to fit spectral energy distribution templates at both emission peaks. The best-fitting templates have extinctions of A{sub V} = 18 and A{sub V} = 9 toward the main and secondary emission peak and we estimated a color temperature of 68 K at both peaks from the 31 {mu}m and 37 {mu}m measurement. At the emission peaks the estimated dust masses are on the order of 10{sup 4} M{sub Sun }.
OSTI ID:
22047903
Journal Information:
Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 2 Vol. 749; ISSN 2041-8205
Country of Publication:
United States
Language:
English

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