From protostellar cores to disk galaxies - Zurich - 09/2007 S.Walch, A.Burkert, T.Naab Munich University Observatory S.Walch, A.Burkert, T.Naab Munich.
Most Stars Are Single ! C. J. Lada ApJ, 640, L63 (2006) 1.From observations: a low binary fraction for late-type stars 2.2/3 of all disk MS stellar systems.
Randolf Klein SOFIA – USRA/NASA Ames July 2014 AASTCS 4: Workshop on Dense Cores - Monterey, CA Issues with SED Fitting, PMS Tracks, and the Birthline.
A Search For Fragmentation in Starless Cores with ALMA Scott Schnee (NRAO) Hector Arce, Tyler Bourke, Xuepeng Chen, James Di Francesco, Michael Dunham,
Randolf Klein SOFIA – USRA/NASA Ames July 2014 AASTCS 4: Workshop on Dense Cores - Monterey, CA
Dust cycle through the ISM Francois Boulanger Institut d ’Astrophysique Spatiale Global cycle and interstellar processing Evidence for evolution Sub-mm.
ARE MAGNETIC FIELDS AND OUTFLOWS ALIGNED IN PROTOSTELLAR CORES? Chat Hull University of California, Berkeley (USA) Radio Astronomy Laboratory 5 February.
ARE MAGNETIC FIELDS AND OUTFLOWS ALIGNED IN PROTOSTELLAR CORES? Chat Hull UC Berkeley, Radio Astronomy Laboratory 10 January 2013 Session 426. Star Formation.
