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Spitzer-IRS Study of the Antennae Galaxies NGC 4038/39

  • Authors: B. R. Brandl, L. Snijders, M. den Brok, D. G. Whelan, B. Groves, P. van der Werf, V. Charmandaris, J. D. Smith, L. Armus, R. C. Kennicutt, Jr., and J. R. Houck

BRANDL et al. 2009 The Astrophysical Journal 699 1982.

  • Provider: AAS Journals

Caption: Figure 11.

False-color IRS spectral map of the H 2 S(3) line in the green and blue channel, and the S(2) line in the red channel in square-root scaling. Bluer colors mean warmer H 2. North is up. The two nuclei and the emission from the clusters in the overlap region are clearly visible. The yellow contour lines indicate the ISOCAM-CVF measurements of the H 2 S(3) line by Haas et al. (2005); the levels are at 39%, 49%, 58%, 68%, 78%, 84%, 90%, and 96% of the maximum intensity (see Figure 2 in Haas et al. 2005).

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