'Crab nebula' presentation slideshows

The Spectrum of Markarian 421 Above 100 GeV with STACEE

The Spectrum of Markarian 421 Above 100 GeV with STACEE. Jennifer Carson UCLA / Stanford Linear Accelerator Center February 2006. Space-based. 10 MeV. 100 MeV. 10 GeV. 100 GeV. 10 TeV. 1 GeV. 1 TeV. 1 MeV. Ground-based. Outline.

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???????. ????????? ???. Supernovae are vast explosions in which a whole star is blown up. They are mostly seen in distant galaxies as `new' stars appearing close to the galaxy of which they are members. They are extremely bright, rivalling, for a few

674 views • 58 slides

Microsoft Large Databases and Grid Computing

Microsoft Large Databases and Grid Computing. Jim Gray Microsoft Research Gray@Microsoft.com http://research.Microsoft.com/~gray 21 May 2003 . About me. in Microsoft research (located in San Francisco) A database researcher IBM, Tandem, DEC, Microsoft Work on Scalable Systems

626 views • 54 slides

The Life Cycle of Stars

The Life Cycle of Stars. From birth, to death , to live, once again. Life Cycle. Very Small Sized Star. Nebula Protostar Brown dwarf. Life Cycle. Eagle Nebula. Protostar. Brown dwarf. Small Sized Star. Nebula Protostar Red Dwarf White Dwarf. Life Cycle. Omega Nebula. Protostar.

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Life of a Star

Life of a Star. Nebula. A cloud of dust and gas in which new stars form. Nebula. Nebula. Star -uses Hydrogen as fuel. Nebula. Star -uses Hydrogen as fuel. Red Giant -uses Helium as fuel. Red giant.

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First Results from VERITAS

First Results from VERITAS. David Hanna McGill University Montreal, Canada. Outline of Presentation. - collaboration - description of the detector telescopes readout trigger construction timeline - 2006-2007 observations Crab Mrk431, Mrk501 LSI+61 303 1ES 1218 M87

459 views • 35 slides

Serge BOUQUET serge.bouquet@cea.fr CEA, DAM, DIF, F - 91297 Arpajon, France and

International Conference on High Energy Density Laboratory Astrophysics - HEDLA - Tallahassee (FL - USA), April 29 - May 04, 2012. SCALING ASTROPHYSICAL RADIATION HYDRODYNAMICS for the LABORATORY. Serge BOUQUET serge.bouquet@cea.fr CEA, DAM, DIF, F - 91297 Arpajon, France and

570 views • 29 slides

???? 07: X-ray Polarimetry Missions

???? 07: X-ray Polarimetry Missions. January 15, 2007 Tsunefumi Mizuno Hiroshima University. M. McConnel "Status and Future Prospects for gamma-ray Polarimetry" and references therein (X-Ray Polarimetry Workshop at SLAC/Stanford, 2004;

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Chapter 11 Simple Harmonic Motion

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298 views • 19 slides

Observation of the Crab Nebula with the MAGIC Telescope

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Neutron Stars

0. Neutron Stars . 0. Gradual compression of a stellar iron core. Radial Structure of a Neutron Star. - Heavy Nuclei ( 56 Fe). - Heavy Nuclei ( 118 Kr); free neutrons; relativistic, degenerate e -. - Superfluid neutrons. 0. Properties of Neutron Stars. Typical size: R ~ 10 km.

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Observations of the AGN 1ES1959+650 with the MAGIC telescope

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Science A-36 Overview and Intro

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Discovery of Temporal Changes in the Torus around PSR B1509-58

Discovery of Temporal Changes in the Torus around PSR B1509-58. Y. Yatsu, N. Kawai, T. Nakamori, & H. Nakajima Tokyo Institute of Technology. Contents of this talk. Introduction Data Analysis and Results Discussion Conclusion. Temporal studies of PWNe.

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First Observations with the MAGIC telescope

First Observations with the MAGIC telescope. Ester Aliu for the MAGIC collaboration. International School of CosmicRay Astrophysics, Erice 2nd-13th July 2004. Introduction. MAGIC is in commissioning phase until October 2004.

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High Sensitivity Balloon-Borne Hard X-Ray/Soft Gamma-Ray Polarimeter PoGOLite

High Sensitivity Balloon-Borne Hard X-Ray/Soft Gamma-Ray Polarimeter PoGOLite. November 2 nd , 2007 IEEE Nuclear Science Symposium Tsunefumi Mizuno (Hiroshima Univ.) for PoGOLite Collaboration Hiroshima Univ., Tokyo Institute of Technology, ISAS/JAXA, Yamagata Univ. (Japan);

253 views • 12 slides

When a Standard Candle Flickers: Crab Nebula Variations in Hard X-rays

When a Standard Candle Flickers: Crab Nebula Variations in Hard X-rays. Colleen A. Wilson-Hodge (NASA/MSFC). Collaborators.

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Goodman Overview & Status:

Goodman Overview & Status:

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G. Kanbach, A. S?owikowska * , S. Kellner**, H. Steinle

Optical polarization measurements of the Crab. Model: Dyks et al., 2004.

107 views • 1 slides