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Five Star‐forming Cores in the Galactic Ring Survey: A Mid‐Infrared Study

  • Authors: Kathleen E. Kraemer, James M. Jackson, Marc Kassis, Lynne K. Deutsch, Joseph L. Hora, Robert Simon, William F. Hoffmann, G. G. Fazio, Aditya Dayal, T. M. Bania, Dan P. Clemens, and Mark H. Heyer

Kraemer et al. 2003 The Astrophysical Journal 588 918.

  • Provider: AAS Journals

Caption: Fig. 5.

Mid‐IR emission from G45.45. The compact component [FSH98] MIR 1 contributes roughly 10% of the flux at both 12.5 (upper left; ﹩1< F< 20﹩ mJy pixel−1) and 20.6 μm (upper right; ﹩6< F< 58﹩ mJy pixel−1). Color temperature (lower left; ﹩110< T_{d}< 150﹩ K, contours at 110, 115, 120, 125, 130, and 140 K) and opacity (lower right; ﹩0.1< \tau _{12.5}< 17.8\times 10^{-3}﹩, contours at 0.5, 1, 2, 4, 6, and ﹩8\times 10^{-3}﹩) maps are also shown. Asterisks in the 12.5 μm map show the positions of the near‐IR sources found by Feldt et al. (1998).

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