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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. 18.

Location of the OB star candidates. Left: Location of OB star candidates within 8﹩\arcmin﹩ of the cluster center noted on a 2MASS K‐band image. The circle indicates 200﹩\arcsec﹩ from the cluster center. The box indicates the VLT field shown in the panel to the right. Right: Location of OB star candidates within 1﹩\farcm﹩25 of the cluster center overlaid on the VLT Ks‐band image. The numbers indicate the X‐ray source number, except in the case of the two VLT‐only sources. To avoid clutter, only the arcseconds of declination are listed for the VLT sources.

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