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low-z analogs for high-z star forming galaxies

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Herschel/PACS spectra of [C II] in <strong>low</strong>-z <strong>galaxies</strong> from SHINING key project:<br />

[C II] deficit at <strong>high</strong> L_IR still seen, exists in other far-IR lines as well.<br />

May get <strong>low</strong>er scatter by plotting against L_IR / M(H2) -<br />

if both ratios are related to density this is sensible.<br />

Gracia-Carpio+ 2011

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