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Join us in Moscow on June 7, 2013, for a stellar astrophysics colloquium outlining magnetic fields, pulsations, abundance analysis, stellar properties, and evolutionary trends. Experts will present new observations, theoretical models, and insights into stellar evolution on the HR diagram.
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Colloquium Resume in outline form Moscow, 7 June 2013
I - Magnetic Fields • A.Overview • Romanyuk, Matthews, Kochukhov, Lignieres. B. Surface, external Alecian, Schoeller, ud-Doula Naze, Robrade C. Methods, origin, theory Arlt, Lau, Rusomarov
II - Pulsations, variability A. New Observations Uytterhoeven, Antoci Mowlavi, Sachkov Balona B. Theory Saio
III - Abundances A. General 1. Results Przybilla, Teker 2. Methods Shulyak, Sitnova, Tsymbal B. Spots Lueftinger, Korhonen Krticka (theory, simulation) C. Stratification Ryabchikova D. Diffusion Landstreet, Staritsin
IV - Properties A. Structure (Size, Shape) Perrault B. Binarity, multiplicity North, Griffin C. Rotation Mathys, Royer, Mikulasek D. Environment 1. Galactic clusters Fossati, Kilcoglu 2. Galaxies Netopil, Urbaneja
V - On the HR Diagram, Evolution A. Disks D’Angelo, Thureau, Grinin 1. planets – Mkrtician B. Herbig Ae/Be Alecian C. Massive stars 1. Winds, x-rays, non-thermal Robrade 2. Valyavin
On the HR Diagram, Evolution (continued) D. Evolutionary changes Semenko E. Supergiants Urbaneja F. White Dwarfs Valyavin
The End Thanks