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The top documents tagged [binary companion]
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binary companion
1 To Be or Not to Be: The Mysteries of Disk Formation Around Rapidly Spinning Be Stars Douglas R. Gies Department of Physics and Astronomy Center for High.
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THE CANNONBALL MODEL AND SHORT HARD BURSTS Arnon Dar 44 th Rencontre De Moriond, La Thuile, Italy, February 1-8, 2009 Based on work done in collaboration.
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Understanding the Evolution of Close Binary Systems With Radio Pulsars
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Magnetars: SGRs and AXPs. Magnetars in the Galaxy ~7 SGRs, ~12 AXPs, plus candidates, plus radio pulsars with high magnetic fields (about them see arXiv:
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Chapter 21 Stellar Explosions. 21.1Life after Death for White Dwarfs 21.2The End of a High-Mass Star 21.3Supernovae Supernova 1987A 21.4The Formation.
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1. accretion disk - flat disk of matter spiraling down onto the surface of a star. Often from a companion star.
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Stellar Explosions. Introduction Life after Death for White Dwarfs The End of a High-Mass Star Supernovae Supernova 1987A The Crab Nebula in Motion The.
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1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If.
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What is Dark Energy? Josh Frieman Fermilab and the University of Chicago.
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1 TORAH LIGHT MINISTRIES P.O. Box 2500 OROVILLE WA 98844 The SIGN and the Flood: Lesson #4.
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What is Dark Energy?
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White Dwarf Stars
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