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Classical and recurrent nova models
(2011)
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Remarkable progress in the understanding of nova outbursts has been achieved
through combined efforts in photometry, spectroscopy and numerical simulations. According to the thermonuclear runaway model, novae are powered ...
Computer simulations using implicit Lagrangian hydrodynamics in 3D
(2011)
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The method known as Smoothed Particle Hydrodynamics (SPH) is an important tool in
modern numerical Astrophysics. It has been extensively used to simulate a large number
of systems ranging from planets to clusters of ...
Population Synthesis of Post-Common Envelope White-Dwarf-Main-Sequence Binaries in the Sloan Digital Sky Survey
(Astronomical Society of the Pacific Conference Series (ASP), 2011)
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