Fig. 14 from X‐Ray and Infrared Point Source Identification and Characteristics in the Embedded, Massive Star‐Forming Region RCW 38

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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. 14.

Hydrogen column as derived by X‐ray spectral fits vs. derived NIR extinction. The line is the best‐fit line passing through the origin ﹩N_{\mathrm{H}\,}=A_{V}\left(2.0\times 10^{21}\right)﹩ cm⁻².

Other Images in This Article

Copyright and Terms & Conditions