CCAT

Formation and Development of Molecular Clouds –
prospects for high resolution spectroscopy with CCAT

2011 October 5–7, Cologne

 

  Website, Poster, and Program Participants
     
 
Presentations
 
     
 
Jason Glenn, U Colorado
 
Mark Heyer, U Massachusetts, &
Robert Simon, U Köln
  Submm and IR studies of molecular regions in the Magellenic clouds
Monica Rubio, U Chile
 
Andy Pon, U Victoria
 
Sergio Molinari, INAF-IFSI Rome
 
Alexi Kritsuk, UC San Diego
 
Volker Ossenkoppf, U Köln
 
Akria Endo, TU Delft
 
Fredrich Wyrowski, MPIfR Bonn
 
John Bally, U Colorado
 
Fabrice Herpin, U Bordeaux
 
Laurent Pagani, Obs Paris
 
Simon Glover, ITA-ZAH Heidelberg
 
Paul Goldsmith, JPL
 
Nicola Schneider, CEA Saclay
 
Doug Johnstone, HIA - U. Victoria
 
Andrey Baryshev, SRON
 
John Carpenter, Caltech
  Using high resolution observations as a probe of prestellar core dynamics Hal Yorke, JPL
  Embracing structural diversity in wide field CCAT maps Jens Kauffmann, JPL
  New flavours in galactic surveys: HOPS and MALT Andrew Walsh, James Cook ULarge
  Characterization of cloud structure Phillipe André, CEA Saclay
  Zeeman observations towards high mass star forming regions using CCAT Hiroko Shinnaga, Caltech
  High resolution wide band spectrometers for large heterodyne arrays Bernd Klein, MPIfR Bonn
  Signatures of molecular cloud formation Clare Dobbs, MPE Garching
  The earliest phases of OB star formation revealed by the Herschel key program HOBYS Martin Hennemann, CEA Saclay
  Filamentary structures traced by IRDCs Gary Fuller, U Manchester
  Molecular gas, dust, and star formation in nearby galaxies Fabian Walter, MPIA Heidelberg
  2 mm ultradeep field observations Johannes Staguhn, GSFC & Johns Hopkins U
  Prospects for high resolution spectroscopy with CCAT Maryvonne Gerin, ENS Paris
  Densitometry and thermometry of starburst galaxies Jeff Mangum, NRAO
  Lines at THz frequencies Rene Plume, U Calgary
  Large high resolution array development Urs Graf, U Köln
  SOFIA and CCAT Hans Zinnecker, DSI - U Stuttgart
  Summary

Paul Goldsmith, JPL

Presentations © 2011 by individual presenters. Format: pdf.