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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. 12.

Composite J‐ (blue), H‐ (green), and Ks‐ (red) band VLT NIR image of RCW 38. The overexposed bright star is the O5 star IRS 2, and the overexposed ﹩\textsf{X}﹩‐shaped nebulosity at ~﹩08^{\mathrm{h}\,}59^{\mathrm{m}\,}04^{\mathrm{s}\,}﹩, ﹩-47^{\circ }30^{\prime }40^{\prime \prime }﹩ near the center of the image is the IRS 1 ridge (Smith et al. 1999). The gray‐scale version of this figure is only the Ks‐band image.

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