A Correlation Between Surface Densities of Young Stellar

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Most Local Star Formation is Clustered, Megeath et al. in prep. Lada & Lada 2003 Gutermuth et al. 2009 Bressert et al. in prep. But Not Dense Incomplete Check out Poster (DP7) and talk! Nearly all star formation within 500 pc! Over 7000 YSOs!
Nearby clusters are not spherical, but often elongated and clumpy. Red: > 100 pc -2 Blue: 10 - 100 pc -2 Green: 1 - 10 pc -2 Surface Density Maps of Infrared-Excess Sources Allen et al. 2007
Page 1 and 2: A Star and Gas Surface Density Corr
Page 3: A Few Terms Explained... YSO - Youn
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 and 14: Gas Poor (YSO Rich?): Cep OB3b Clus
Page 15 and 16: Circles: c2d cloud-integrated value
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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