carma large area star formation survey pi: lee mundy, university of maryland
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CARMA Large Area Star formation Survey PI: Lee Mundy, University of Maryland Co-I: Shaye Storm, University of Maryland (thesis work) Perseus : NGC 1333, Barnard 1, L1451 Serpens : Serpens Main, Serpens South. CarmaOrion PI: John Carpenter, Caltech 1 sq. degree of Orion A - PowerPoint PPT Presentation
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CARMA Large Area Star formation SurveyPI: Lee Mundy, University of MarylandCo-I: Shaye Storm, University of Maryland (thesis work)
Perseus: NGC 1333, Barnard 1, L1451 Serpens: Serpens Main, Serpens South
CarmaOrionPI: John Carpenter, Caltech
1 sq. degree of Orion A (not a member, but happy to advertise!)
Spatial scales from ~0.01 pc – 7 pc Multiple molecular lines to study structure and
kinematics of star forming gas
N2H+ J=1-0 N2H+ vlsr
9.5’
15’
0.65 pc1
pc
J, H, K
Cloud structure formation – the role of turbulence and magnetic fields
Star cluster formation – the connection between dense cores and the IMF
Serpens Main
Orion A
PerseusBarnard 1
Stop by the poster!
0.5
pc
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