A Correlation Between Surface Densities of Young Stellar

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You are entering the Speculation Zone!! My apologies for the ad hoc presentation; this was inspired by yesterday's excellent SF Law breakout session! !(large scale) = Integral ( !(small scale) * dA ) / A We can measure the area distribution function of !(small scale)!
Area distributions of Surface Densities in MonR2 Cloud scale integration moves SF law index from ~2 to ~1.3.
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 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: YSO Evolutionary State Ratio Maps M

A Correlation Between Surface Densities of Young Stellar

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