Fig. 11 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. 11.

Histogram showing X‐ray luminosity distribution in RCW 38. The solid line shows the distribution of 365 candidate cluster members with spectral fits. The dotted line shows the expected full distribution of X‐ray luminosities assuming a lognormal distribution (after Feigelson et al. 2005).

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