'Dark matter halo' diaporamas de présentation

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GEARS Workshop Galaxies Sarah Higdon

GEARS Workshop Galaxies Sarah Higdon. Galaxy Evolution. We will test some of the GEARS Galaxy Evolution Unit. There are two goals 1: For everyone to be comfortable with presenting the material in the classrooms.

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Galactic Matter and Dark Matter

Galactic Matter and Dark Matter. Ramanath Cowsik and Benjamin Burch Physics Department McDonnell Center for the Space Sciences Washinton University in St. Louis, USA 63130 WHEPP XII: Mahabaleshwar , India January 4-5 Thanks to Professor Sreerup Raychaudhuri & Professor Utpal Sarkar.

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Chapter 5: Cosmic foundations for origins of life

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Units to be covered:77-82

Units to be covered:77-82 . Also please send suggestions for the topics to be covered by my next lecture on Dec. 10. This lecture is going to cover exciting developments in Astrophysics and Cosmology not covered by your textbook. My mail is lazarian@astro.wisc.edu.

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The Hamming Seminars

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The Baryon Induced Transformation of CDM Halos

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The Milky Way Galaxy

The Milky Way Galaxy. 1/30/03. The Milky Way. Brief History Morphology - what are the components of the Galaxy? The Galactic Rotation The Galactic Center. Brief History. What is the Shape of the Milky Way?.

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Chania, Crete, August 2004 “The environment of galaxies”

Pierre-Alain Duc Recycling in the galaxy environment. F. Bournaud J. Braine U. Lisenfeld P. Amram P. Weilbacher. Chania, Crete, August 2004 “The environment of galaxies”. Looking between galaxies…. @ Gregg & West. Stars in the intracluster medium. Diffuse light

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Vienna 12/04/06

Three-dimensional hydrodynamical simulations of ISM pollution by type Ia and II supernovae in forming dwarf spheroidal galaxies.

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Nubecula Major

Timewaste-o-Vision. IN GLORIOUS. Nubecula Major. Adric Riedel. Outline. Basic Facts Discovery Morphology Its place in the Local Group Relation to the Small Magellanic Clouds As compared to other galaxies The Past and Future of the LMC Dark Nebulae Terminal spiral into Milky Way

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Asymmetry of the Milky Way

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Constraining Galactic Halos with the SZ-effect

Constraining Galactic Halos with the SZ-effect. by Naureen Goheer, University of Cape Town based on a collaboration with Kavilan Moodley (UKZN). Galaxy morphology. spirals much better understood, focus on them. rich in gas and dust. 90%. 10%.

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Galaxy Formation and Evolution Open Problems

Galaxy Formation and Evolution Open Problems. Alessandro Spagna Osservatorio Astronomico di Torino Torino, 18 Febbraio 2002. Galaxy Structure. Flat disk : 10 11 stars (Pop.I) ISM (gas, dust) 5% of the Galaxy mass, 90% of the visible light Active star formation since 10 Gyr.

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Cosmological Structure Formation A Short Course

Cosmological Structure Formation A Short Course. II. The Growth of Cosmic Structure Chris Power. Recap. The Cold Dark Matter model is the standard paradigm for cosmological structure formation .

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Introductory remarks Outline of physics concepts Description of the experiment Results

CDMS (Cryogenic Dark Matter Search) Long Duong (University of Minnesota) Trinity School Seminar Jan 14, 2004. Introductory remarks Outline of physics concepts Description of the experiment Results. ~ 40 physicists/students from 8 institutions work on CDMS

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The Milky Way

The Milky Way Structure of the Milky Way The Milky Way Components of the Milky Way Disk Population I stars Open clusters HII regions Bulge Population II stars Halo Globular clusters Omega Centauri Stellar Populations M100 Finding Our Place Globular Clusters evenly distributed

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The ages and metallicities of Hickson Compact Group galaxies.

The ages and metallicities of Hickson Compact Group galaxies. Rob Proctor Swinburne University of Technology May 2005. Collaborators: Duncan Forbes (Swinburne University of Technology) George Hau (Durham) Mike Beasley (Santa Cruz). Aim and Outline. Aim:

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