low-z analogs for high-z star forming galaxies
low-z analogs for high-z star forming galaxies
low-z analogs for high-z star forming galaxies
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[O I] / [C II] ratio (density or ionization) is correlated with f_60 / f_100 (dust temperature)<br />
Correlation known from ISO data (Malhotra et al 2001). The disky LIRGs are cooler than<br />
ULIRGs, and shifted to <strong>low</strong>er [O I] or warmer dust compared to the <strong>low</strong>er-luminosity SFGs.
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