'Low mass star formation' presentation slideshows

Star Formation in Context

Star Formation in Context. Neal Evans University of Texas at Austin. Context. Individual star formation in detail Initial conditions and early evolution Formation and evolution of disks Provides the context for planet formation Massive, clustered star formation Details less accessible

970 views • 60 slides

Star and Planet Formation

Star and Planet Formation. Neal Evans The University of Texas at Austin. Star Formation in Galaxies. Antennae: galaxy merger. Visible (HST) shows copious star formation, but misses the main show. Most intense star formation in obscured region traced by CO. CO(1-0): OVRO.

784 views • 55 slides

Star and Planet Formation

Star and Planet Formation. Neal Evans The University of Texas at Austin. Star Formation in Galaxies. Antennae: galaxy merger. Visible (HST) shows copious star formation, but misses the main show. Most intense star formation in obscured region traced by CO. CO(1-0): OVRO.

572 views • 55 slides

Only on the largest cosmological scales is astronomy simple!

601 views • 47 slides

Science With ALMA

Science With ALMA. T. L. Wilson European ALMA Project Scientist, and Interim JAO Project Scientist. Bilateral ALMA + ALMA Compact Array (in lower right). Location Chajntantor Plateau at 5000m in northern Chile. ALMA. ALMA Science Drivers. Key drivers: Detect the Milky Way at z=3

594 views • 38 slides

Star and Planet Formation

Star and Planet Formation. Sommer term 2007 Henrik Beuther & Sebastian Wolf. 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation transfer (H.B.) 30.4 Gravitational collapse & early protostellar evolution I (H.B.)

374 views • 27 slides

Star and Planet Formation

Star and Planet Formation. Sommer term 2007 Henrik Beuther & Sebastian Wolf. 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation transfer (H.B.) 30.4 Gravitational collapse & early protostellar evolution I (H.B.)

370 views • 27 slides

Star and Planet Formation

Star and Planet Formation. Sommer term 2007 Henrik Beuther & Sebastian Wolf. 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation transfer (H.B.) 30.4 Gravitational collapse & early protostellar evolution I (H.B.)

273 views • 27 slides

Chemical evolution from cores to disks

375 views • 24 slides

Introduction Molecular clouds are generally: Self-gravitating, Magnetized, Turbulent,

The Structur and Evolution of Molecular Clouds: From Clumps to Cores to the IMF J.P.Williams; L. Blitz; C.F.McKee. Introduction Molecular clouds are generally: Self-gravitating, Magnetized, Turbulent, Compressible fluids What do we want to understand in this paper?

201 views • 12 slides

Conference Summary Outstanding questions: a personal view

Conference Summary Outstanding questions: a personal view. Zooming in on Star Formation , Nafplio, June 14 , 2019. Galactic Scale Star Formation. What we know for sure now: Feedback, and vertical pressure ( im -)balance is crucial

209 views • 9 slides