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SOFIA Far-infrared Imaging Polarimetry of M82 and NGC 253: Exploring the Supergalactic Wind

  • Authors: Terry Jay Jones, C. Darren Dowell, Enrique Lopez Rodriguez, Ellen G. Zweibel, Marc Berthoud, David T. Chuss, Paul F. Goldsmith, Ryan T. Hamilton, Shaul Hanany, Doyal A. Harper, Alex Lazarian, Leslie W. Looney, Joseph M. Michail, Mark R. Morris, Giles Novak, Fabio P. Santos, Kartik Sheth, Gordon J. Stacey, Johannes Staguhn, Ian W. Stephens, Konstantinos Tassis, Christopher Q. Trinh, C. G. Volpert, Michael Werner, and Edward J. Wollack

2019 The Astrophysical Journal Letters 870 L9.

  • Provider: AAS Journals

Caption: Figure 1.

M82 maps of color temperature (left) and column density (right). The temperature contours start at 20 K and increase in 2 K increments. The column density contours start at ﹩\mathrm{log}\left(N({\rm{H}}+{{\rm{H}}}_{2})\right)=21﹩ and increase in increments of 0.2.

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