A Correlation Between Surface Densities of Young Stellar

ePAPER READ

DOWNLOAD ePAPER

conference.astro.ufl.edu

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

START NOW

YSO Evolutionary State Ratio Maps<br />

MonR2<br />

Class II >> Class I<br />

Class II ~ Class I<br />

Cep OB3

Recommendations
Info

MonR2 Star-Gas Evolution Maps High !(YSOs) / ! 2 (gas) Low !(YSOs) / ! 2 (gas) log{!(YSOs) / ! 2 (gas)} ~ -3.3 MonR2 is largely colorless! Cep OB3 Cep A Cep C Cep OB3 is “motley”, but embedded clusters are colorless!

YSO Evolutionary State Ratio Maps MonR2 Class II >> Class I Class II ~ Class I Cep OB3

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: -5 -4 -3 -2 -1 Log {!(YSOs) / ! 2 (
Page 23 and 24: Area distributions of Surface Densi

A Correlation Between Surface Densities of Young Stellar

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?