Fig. 4 from X‐Ray and Infrared Point Source Identification and Characteristics in the Embedded, Massive Star‐Forming Region RCW 38

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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. 4.

Left: Position plot of all probable X‐ray cluster members as determined by quartile analysis. Right: Position of nonmembers. A density analysis shows that this distribution is uniform.

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