Can Photo-Evaporation Trigger Planetesimal Formation? Henry Throop John Bally SWRI Univ.Colorado / CASA DPS 12-Oct-2004.
Cumber01.ppt 30.5.2001 Thomas Henning Max-Planck-Institut für Astronomie, Heidelberg Protoplanetary Accretion Disks From 10 arcsec to 10 -3 arcsec HST.
Jets and Disks in Young Stellar Objects Introduction Jets and disks in low-mass young stellar objects The search for jets and disks in massive young stars.
UNIT 5 BASKETBALL REVIEW
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Dissection of a Cold, Infalling High-Mass Star-Forming Core
Chapter 13: Chapter 13: The Deaths of Stars The Helix Nebula.
Accretion in Binaries Two paths for accretion –Roche-lobe overflow –Wind-fed accretion Classes of X-ray binaries –Low-mass (BH and NS) –High-mass (BH and.
From Pre-stellar Cores to Proto-stars: The Initial Conditions of Star Formation PHILIPPE ANDRE DEREK WARD-THOMPSON MARY BARSONY Reported by Fang Xiong,
A massive disk around the intermediate-mass young star AFGL 490 ? Katharina Schreyer (AIU Jena, Germany) Thomas Henning (MPIA Heidelberg, Germany) Floris.
Observing Star-Formation From the Interstellar Medium to Star-Forming Cores On-Line Version, 1999 Alyssa A. Goodman Harvard University Department of Astronomy.
DARS, October 9, 2008 Chemical evolution in the MW Observational evidence Birgitta Nordström Niels Bohr Institute.