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X‐Ray and Infrared Point Source Identification and Characteristics in the Embedded, Massive Star‐Forming Region RCW 38

  • Authors: Scott J. Wolk, Bradley D. Spitzbart, Tyler L. Bourke, and João Alves

Wolk et al. 2006 The Astronomical Journal 132 1100.

  • Provider: AAS Journals

Caption: Fig. 1.

Left: Bulk of ACIS‐I image of RCW 38 at low resolution. Right: Matching field in a 2MASS K‐band image. The FOV in these figures is ﹩16^{\prime }\times 16^{\prime }﹩. Regions of interest are identified. The ellipses near the core are the "common background regions" used for sources in the core as discussed in § 2.2. At 1.7 kpc, ﹩121^{\prime \prime }=1\ \mathrm{pc}\,﹩.

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