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YOUNG STELLAR OBJECTS IN THE MASSIVE STAR-FORMING REGION W49

  • Authors: G. Saral, J. L. Hora, S. E. Willis, X. P. Koenig, R. A. Gutermuth, and A. T. Saygac

2015 The Astrophysical Journal 813 25.

  • Provider: AAS Journals

Caption: Figure 2.

Left panel shows a color image of the entire mosaic in the Spitzer IRAC bands (blue: 3.6 μm, green: 4.5 μm, red: 8.0 μm). The dashed line denotes the Galactic plane. The field shown by the dashed gray box is where we performed the clustering analysis, which is shown in detail in the right panel. The size scales in pc assume a distance to W49 of 11.1 kpc.

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