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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. 9.

Histogram of derived plasma temperatures for each cluster member. Fits for 188 sources fitted with one‐temperature Raymond‐Smith plasma are indicated by the open histogram. The filled histogram represents the high‐temperature component of the two‐temperature fits. The hatched histogram represents the low‐temperature component from these fits. The bins are 0.25 keV wide.

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