Accretion High Energy Astrophysics [email protected]
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.
Composite colliding winds (CWo - orbiting; CWc - concentric; CWb - binary) and Seaquist, Taylor and Button (STB) model of HM Sge (open circle - hot component;
The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different.
Measuring the Mass of Stars Physics 113 Goderya Chapter(s): 9 Learning Outcomes:
Extra Solar Planets
Hee-Won Lee ARCSEC and Dept. of Astronomy Sejong University 2010 August 26.
X-Ray Binary Light-Curve Analysis in optical and x-ray or “the ‘crazy’ LMXB (low mass x-ray binary) EXO 0748-676“ Trainee: Alexander Kolodzig Origin: HU.
Cataclysmic Variable Stars
ASTR 1102-002 2008 Fall Semester
Extra Solar Planets Just some introductory materials. A very fast moving field. My favorite website: .
Near IR Spectroscopy of Symbiotic Stars and Young Planetary Nebulae
