'Virial theorem' presentation slideshows

Ch121a Atomic Level Simulations of Materials and Molecules

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Ralph Pudritz McMaster University, Origins Institute

511 views • 41 slides

678 views • 40 slides

Star and Planet Formation

Star and Planet Formation. Sommer term 2007 Henrik Beuther & Sebastian Wolf. 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation transfer (H.B.) 30.4 Gravitational collapse & early protostellar evolution I (H.B.)

396 views • 28 slides

Star and Planet Formation

Star and Planet Formation. Sommer term 2007 Henrik Beuther & Sebastian Wolf. 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation transfer (H.B.) 30.4 Gravitational collapse & early protostellar evolution I (H.B.)

282 views • 28 slides

Galaxy Characteristics

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The Large Scale Structure of the Universe

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The Large Scale Structure of the Universe

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X-RAY CLUSTERS IN CONFORMAL GRAVITY

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PHY 7 11 Classical Mechanics and Mathematical Methods 9-9:50 AM MWF Olin 107

PHY 7 11 Classical Mechanics and Mathematical Methods 9-9:50 AM MWF Olin 107 Plan for Lecture 13: Finish reading Chapter 6 Virial theorem Canonical transformations Hamilton-Jacobi formalism. Virial theorem ( Clausius ~ 1860). Note that this implies that the motion is bounded.

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Lecture 14

Lecture 14. Star formation. Insterstellar dust and gas. Dust and gas is mostly found in galaxy disks, and blocks optical light. The interstellar medium. Stars are born from this gas and dust, collectively known as the interstellar medium .

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Physics of Fusion power

Physics of Fusion power. Lecture3 : Force on the plasma / Virial theorem. Break-even. The break-even condition is defined as the state in which the total fusion power is equal to the heating power Note that this does not imply that all the heating power is generated by the fusion reactions.

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Physics 133: Extragalactic Astronomy and Cosmology

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Cosmology and Clusters: The Coma Cluster

Cosmology and Clusters: The Coma Cluster. Ken Zhao and Arthur Su Newton North High School Chandra Astrophysics Institute May 12, 2007. Outline. Introduction Cosmology and Clusters Questions What is the MASS of clusters? In particular, the Coma Cluster Methods/Data

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Physics 133: Extragalactic Astronomy and Cosmology

Physics 133: Extragalactic Astronomy and Cosmology. Lecture 10; February 12 2014. Previously:. How do we measure cosmological parameters? The Hubble constant Measuring v (peculiar velocities) Measuring D (the cosmic distance ladder) Cosmography Luminosity distance and standard candles

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Stellar Structure

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Stellar Structure

104 views • 10 slides