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Big Data, Space Weather and cognitive visualization Проблема больших объемов данных в космической погоде и когнитивная визуализация
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.
Evolution of a Powerful Radio Loud Quasar 3C186 and its Impact on the Cluster Environment at z=1 Aneta Siemiginowska Harvard-Smithsonian Center for Astrophysics.
Can a double component outflow explain the X-ray and Optical Lightcurves of GRBs? Massimiliano De Pasquale 1 P. Evans 2, S. Oates 1, M. Page 1, S. Zane.
Kieran O’Brien ESO, Paranal Science Operations (UCSB, Santa Barbara, California) Vik Dhillon (Sheffield, UK), Tom Marsh (Warwick, UK), Derek Ives (UKATC,
The Solar System Ingredients? ● The Sun ● Planets ● Moons and Rings ● Comets ● Asteroids (size > 100 m) ● Meteoroids (size < 100 m) ● Kuiper Belt ● Oort.
15 The Milky Way More than just a candy bar.. 15.
1 Detecting Supernova Neutrinos X.-H. Guo Beijing Normal University.
Physics of magnetically dominated plasma: dynamics, dissipation and particle acceleration Maxim Lyutikov (UBC) Cracow, June 2006.
The multi-wavelength polarization VLBI structure of 3 BL Lacertae objects Vladislavs Bezrukovs, Dr. Denise Gabuzda EVN 8 th Symposium 26 – 29 September,
Instrumental Chemistry Chapter 7 and 8 Optical Spectroscopy- Components and Introduction.
