Our Place in the Cosmos Lecture 11 Understanding Stars - the H-R Diagram.
1)Are disks predicted? Theories of HM SF 2)Are disks observed? Search methods 3)Observational evidence disks VS toroids 4)Open questions and the future:
Angular Momentum and the Formation of Stars and Black Holes Richard B. Larson Yale University.
Nathan Mayne Empirical Studies of the Secular Evolution of Pre-Main-Sequence Stars Background picture: Collaborators: Tim.
Observations with MOST Pulsations in Wolf-Rayet stars : André-Nicolas Chené (NRC/HIA/CGO) Anthony F. J. Moffat (Université de Montréal) André-Nicolas Chené.
Fy12 astronomy
Science with the Herschel far-infrared & submillimeter space telescope
The lagoon nebula_and_its_vicinity
Deriving direct mass measurements of black holes in ULXs Jeanette Gladstone, T. Roberts, C. Copperwheat, A. Goulding, C. Heinke, A Swinbank, T. Cartwright,
Theories of Massive Star Formation Ian A. Bonnell University of St Andrews.
Star Clusters in the Galactic Center Sgr A* at 30 Workshop Green Bank W.Va March 25, 26, 2004 Donald F. Figer STScI.
Margaret M. Hanson, PhD Associate Professor of Physics.
