Fig. 9 from [Si II], [Fe II], [C II], and H2 Emission from Massive Star‐forming Regions

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

[Si II], [Fe II], [C II], and H₂ Emission from Massive Star‐forming Regions

Kaufman, Wolfire, & Hollenbach 2006 The Astrophysical Journal 644 283.

Caption: Fig. 9.

H₂ 0–0 S(2)/0–0 S(0) line intensity ratio as a function of hydrogen nucleus density n and FUV radiation field G₀.