'Stellar mass black holes' diaporamas de présentation

Chapter 14: Black Holes: Matters of Gravity

Chapter 14: Black Holes: Matters of Gravity. Special Relativity Time Dilation Length Contraction General Relativity Curved Spacetime Swartzschield Black Holes Kerr Black Holes Worm Holes. Stellar Mass Black Holes Intermediate Range Black Holes Super-massive Black Holes

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What Happens Close to a Black Hole ?

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Active Galaxies and Mathematical Models

Active Galaxies and Mathematical Models. Fill in your information here. The NASA Educator Ambassador Program at SSU. You should modify this slide to fit you. Swift. GLAST. XMM-Newton. What is GLAST?. GLAST: Gamma-Ray Large Area Space Telescope Planned for launch in 2007

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Lecture 18 Black Holes (cont)

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Ultraluminous X-ray Sources (ULXs) and Intermediate Mass Black Holes (IMBHs) (For Journal Club)

Ultraluminous X-ray Sources (ULXs) and Intermediate Mass Black Holes (IMBHs) (For Journal Club). J. F. Wu Tsinghua Center for Astrophysics Department of Physics, Tsinghua University. Main References.

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Credit: A. Broderick & E. Mer

Measuring the Spins of Stellar-Mass Black Holes by Fitting the X-ray Continuum Spectrum Jeff McClintock. Credit: A. Broderick & E. Mer. Probing Strong Gravity Near Black Holes Prague: 2010 February 15-18. Our Team. Jeff McClintock Ramesh Narayan

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Astronomy 1020-H Stellar Astronomy Spring_2014 Day-38

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Astronomy 1020 Stellar Astronomy Spring_2014 Day-38

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Astronomy Division C

Science Olympiad. Astronomy Division C. Guidelines. Description: Students will demonstrate an understanding of the basic concepts of mathematics and physics relating to stellar evolution and Type II Supernova. A team of up to: 2 Approximate Time: 50 minutes. Guidelines.

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Astronomy Division C

Science Olympiad. Astronomy Division C. Guidelines. Description: Students will demonstrate an understanding of the basic concepts of mathematics and physics relating to stellar evolution and Type II Supernova. A team of up to: 2 Approximate Time: 50 minutes. Guidelines.

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Today in Astronomy 102: observations of stellar-mass black holes

Today in Astronomy 102: observations of stellar-mass black holes. Summary of distinctive features of celestial black holes. The search for stellar-mass black holes: X-ray and ? -ray emission. Mass from orbital motion: the Doppler effect.

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Topics to be covered and reviewed in this Talk

Topics to be covered and reviewed in this Talk. What is a dwarf galaxy, as opposed to a star cluster?

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Today in Astronomy 102: observations of stellar-mass black holes

Today in Astronomy 102: observations of stellar-mass black holes. Summary of distinctive features of celestial black holes. The search for stellar-mass black holes: X-ray and ? -ray emission. Mass from orbital motion: the Doppler effect.

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The evolution and collapse of BH forming stars

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QSO - m QSO - GRB ANALOGY

QSO - m QSO - GRB ANALOGY. HAVE THE SAME 3 BASIC INGREEDIENTS (M. & Luis Rodriguez, S&T 2002). neutron star. no ?. no. AN UNIVERSAL MAGNETO-HYDRODINAMIC MECHANISM FOR JETS ?. GAMMA-RAY BURSTS. THE MOST ENERGETIC EXPLOSIONS IN THE UNIVERSE.

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QSO - m QSO - GRB ANALOGY

QSO - m QSO - GRB ANALOGY. HAVE THE SAME 3 BASIC INGREEDIENTS (M. & Luis Rodriguez, S&T 2002). neutron star. no ?. no. AN UNIVERSAL MAGNETO-HYDRODINAMIC MECHANISM FOR JETS ?. GAMMA-RAY BURSTS. THE MOST ENERGETIC EXPLOSIONS IN THE UNIVERSE.

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An Overabundance of X-ray Binaries in the Central Parsec of the Galaxy

An Overabundance of X-ray Binaries in the Central Parsec of the Galaxy. Michael Muno (UCLA) with Fred Baganoff (MIT), Eric Pfahl (UVa), Mark Morris, Andrea Ghez, Jessica Lu (UCLA), Geoff Bower (Berkeley), Farhad Yusef-Zadeh, and Doug Roberts (Northestern). We Study the Galactic Center.

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Chandra Science Highlight

Chandra Science Highlight. Evidence for A Swarm of Black Holes in the Galactic Center. Chandra X-ray Observatory ACIS Image.

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