Published April 20, 2012 | Version v1
Journal article

MID-IR FORCAST/SOFIA OBSERVATIONS OF M82

  • 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)

Description

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☉.

Availability note (English)

Available from http://dx.doi.org/10.1088/2041-8205/749/2/L19

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal Letters
Journal Volume
749
Journal Issue
2
Journal Page Range
[6 p.]
ISSN
2041-8205