• DOI:10.1093/pasj/63.sp2.S505
• Corpus ID: 119203790

Diffraction-Limited Subaru Imaging of M 82: Sharp Mid-Infrared View of the Starburst Core*

@article{Gandhi2011DiffractionLimitedSI,
  title={Diffraction-Limited Subaru Imaging of M 82: Sharp Mid-Infrared View of the Starburst Core*},
  author={P Gandhi and Naoki Isobe and Mark Birkinshaw and D. M. Worrall and Itsuki Sakon and Kazushi Iwasawa and Aya Bamba},
  journal={Publications of the Astronomical Society of Japan},
  year={2011},
  volume={63},
  pages={505}
}

• P. Gandhi, N. Isobe, +4 authors A. Bamba
• Published 25 January 2011
• Physics
• Publications of the Astronomical Society of Japan

We present new imaging at 12.81 and 11.7 � m of the central � 40 00 � 30 00 (� 0.7 kpc � 0.5 kpc) of the starburst galaxy M 82. The observations were carried out with the COMICS mid-infrared (mid-IR) imager on the 8.2 m Subaru Telescope, and are diffraction-limited at an angular resolution of <0: 00 4. The images show extensive diffuse structures, including a 7 00 -long linear chimneylike feature and another resembling the edges of a ruptured bubble. This is the clearest view to date of the base of the kpc-scale dusty wind known in this galaxy. These structures do not trace back to a single central point, implying multiple ejection sites for the dust. In general, the distribution of dust probed in the mid-IR anticorrelates with the locations of massive star clusters that appear in the near-infrared. The 10–21 � m mid-IR emission, spatially integrated over the field of view, may be represented by hot dust with temperature of � 160 K. Most discrete sources are found to have extended morphologies. Several radio H II regions are identified for the first time in the mid-IR. The only potential radio supernova remnant to have a mid-IR counterpart is a source which has previously also been suggested to be a weak active galactic nucleus. This source has an X-ray counterpart in Chandra data which appears prominently above 3 keV and is best described as a hot (� 2.6 keV) absorbed thermal plasma with a 6.7 keV Fe K emission line, in addition to a weaker and cooler thermal component. The mid-IR detection is consistent with the presence of strong [Ne II]� 12.81 � m line emission. The broad-band source properties are complex, but the X-ray spectra do not support the active galactic nucleus hypothesis. We discuss possible interpretations regarding the nature of this source.