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The top documents tagged [xray bursts]
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The Physics of Nuclei, Nuclear Matter and Nucleosynthesis Report of the Nuclear Physics Advisory Panel
217 views
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(Recalling the Death of a High-Mass Star…). Neutron stars, although they have 1–3 solar masses, are so dense that they are very small. This image
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Supermassive black holes. 2 Plan of the lecture 1. General information about SMBHs. 2. “Our” certain black hole: Sgr A*. 3. SMBHs: from radio to gamma
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A.What is the EOS? 0. Relationship to energy and to nuclear masses 1. Important questions B. What observables are sensitive to the EOS and
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João Braga
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Binary millisecond X-ray pulsars Department of Physics University College Cork Paul Callanan and Mark Reynolds Alexei Filippenko, Department of Astronomy,
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Today in Astronomy 102: black hole observations, volume 2
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SLAC’s First Step into Space: Status of the USA experiment 5-years after launch
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Mats Lindroos Measuring difficult reaction rates involving radioactive beams: A new approach John D’Auria, Mats Lindroos, Jordi Jose and Lothar Buchmann
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Binary millisecond X-ray pulsars
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Francesca Gulminelli - LPC Caen, France Extended Nuclear Statistical Equilibrium and applications to (proto)neutron stars Extended Nuclear Statistical
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Nuclear Physics in X-ray binaries the rp-process and more Open questions Nuclear physics uncertainties status of major waiting points reaction rates mass
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