A Correlation Between Surface Densities of Young Stellar

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3.6 micron 4.5 micron 8.0 micron YSO Poor (Gas Rich?): Serpens South Filaments N(CII) / N(CI) ~ 1 Gould Belt Legacy Survey – PI Lori Allen Gutermuth et al. 2008 Lots <strong>of</strong> dense gas, but few YSOs! 8.0 micron Class I Class II
Circles: c2d cloud-integrated values 2009 (Galaxy integrated) (HCN, a dense gas tracer) (Individual SF sites in Nearby Galaxies) Assuming Mean YSO age/lifetime <strong>of</strong> 2 Myr Check out Amanda Heiderman's poster (EP20) and talk by Neal Evans!
Page 1 and 2: A Star and Gas Surface Density Corr
Page 3 and 4: A Few Terms Explained... YSO - Youn
Page 5 and 6: Nearby clusters are not spherical,
Page 7 and 8: Class I Class II Stars Form in Mole
Page 9 and 10: A Correlation Between Star and Gas
Page 11 and 12: !(YSOs) (Msun / pc 2 ) A Correlatio
Page 13: Gas Poor (YSO Rich?): Cep OB3b Clus
Page 17 and 18: Conclusions Most stars form in clus
Page 19 and 20: -5 -4 -3 -2 -1 Log {!(YSOs) / ! 2 (
Page 21 and 22: YSO Evolutionary State Ratio Maps M
Page 23 and 24: Area distributions of Surface Densi

A Correlation Between Surface Densities of Young Stellar

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