Mid-IR FORCAST/SOFIA Observations of M82
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 ⊙.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- April 2012
- DOI:
- 10.1088/2041-8205/749/2/L19
- arXiv:
- arXiv:1203.6797
- Bibcode:
- 2012ApJ...749L..19N
- Keywords:
-
- galaxies: individual: M82;
- galaxies: ISM;
- galaxies: starburst;
- infrared: ISM;
- Astrophysics - Cosmology and Nongalactic Astrophysics;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- ApJL in press (ApJ, 749, L19), article also available at at http://stacks.iop.org/2041-8205/749/L19