Fig. 19 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. 19.

X‐ray spectra of two cool white dwarf candidates. These spectra are unusual in their lack of flux above 2.5 keV. They have been fitted with blackbodies with temperatures below 150 eV (histogram), consistent with the emission expected from a degenerate star.

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