Fig. 10 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. 10.

Left: Histogram of ﹩N_{\mathrm{H}\,}﹩ derived through spectral fits of the 209 brightest cluster members. While the distribution is peaked at ﹩2.8\times 10^{22}﹩ cm⁻², at least two cluster members have an order of magnitude more absorption. Right: Histogram of ﹩N_{\mathrm{H}\,}﹩ for the 157 cluster members with <30 counts.

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