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A Correlation Between Surface Densities of Young Stellar

A Correlation Between Surface Densities of Young Stellar

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Deviations from the <strong>Correlation</strong>: Local Evolutionary Differences?<br />

Class II YSOs in gray<br />

Class I YSOs in red<br />

N(CII) / N(CI) is consistently<br />

LOW for Gas Poor<br />

N(CII) / N(CI) is consistently<br />

HIGH for YSO Poor<br />

!(YSOs) (Msun / pc 2 )<br />

2000<br />

200<br />

20<br />

2<br />

0.2<br />

Gas poor<br />

(YSO rich?)<br />

10 100<br />

!(gas) (Msun / pc 2 )<br />

YSO poor<br />

(Gas rich?)

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