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The top documents tagged [stellar winds]
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stellar winds
Stars were originally classified according to their spectra (strength = width of their absorption lines) either from a purely observational perspective.
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Astronomy 535 Stellar Structure Evolution. Course Philosophy “Crush them, crush them all!” -Professor John Feldmeier.
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Star formation simulations -> N=10000……. Cathie Clarke, I.O.A. cf special issue Phil. Trans. Roy. Soc., ed. De Grijs,Ch.3,arXiv:0911.0780.
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1 There and Back Again: Cycles of Activity in Radio Galaxies Stefi Baum and Chris O’Dea Rochester Institute of Technology.
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How well do we understand outflows and accretion on cosmic scales? Romeel Davé.
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This set of slides This set of slides starts the topic of stellar evolution, overview, protostars, main sequence… Units covered: 59, 60, 61.
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A Multiphase, Sticky Particle, Star Formation Recipe for Cosmology Craig Booth Tom Theuns.
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Mike Shara Department of Astrophysics American Museum of Natural History STAR CLUSTER DYNA MIC S Or: BINARY EVOLUTION on STEROIDS.
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Krakow 2010 Galactic magnetic fields: MRI or SN-driven dynamo? Detlef Elstner Oliver Gressel Natali Dziourkevich Alfio Bonanno Günther Rüdiger.
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Solar and Stellar Winds The Sun and other stars are commonly characterized by the radiation they emit. But the past half-century has seen the discovery.
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The Formation of High Mass Stars Richard I. Klein UC Berkeley, Department of Astronomy and Lawrence Livermore National Laboratory Collaborators Mark Krumholz.
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Trends in the Chandra X-Ray Spectra of O and Early B Stars June 24, 2008.
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