1 / 3

CARMA Large Area Star formation Survey PI: Lee Mundy, University of Maryland

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

delta
Download Presentation

CARMA Large Area Star formation Survey PI: Lee Mundy, University of Maryland

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. 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 (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

  2. 9.5’ 0.65 pc N2H+vlsr N2H+ J=1-0 15’ 1 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

  3. Serpens Main Perseus Barnard 1 Orion A 0.5 pc Stop by the poster!

More Related