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Daniel Progas UNLV Home Page GRB and Universe t

Daniel Progas UNLV Home Page GRB and Universe t

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T 90-HR diagram of GRBs. The background orange dots are

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The Afterglows and Redshifts of Swift GRBs

Marianne Vestergaard Dark Cosmology Centre, Copenhagen First Galaxies, Quasars, and GRBs, June

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Fig. 1, Left: X-ray emission (blue), radio emission

Table 2 Observational Criteria for Physically Classifying GRBs

GRBs - UNLV Department of Physics and Astronomy - University of .

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Stellar radio emission in the SKA era: the SCORPIO ... - IRA -

Quasars, black holes and galaxy evolution Clive Tadhunter University of Sheffield 3C273.

Figure 3. (a) E p-E γ,iso diagram of the three samples

Jets from Active Galactic Nuclei: Observations and Models

Ch 1 slides - UNLV Department of Physics and Astronomy

Figure 8. Mass inflow rate at the inner boundary versus time, for seven runs

Simulated 15–150 keV light curves of the pseudo-GRBs obtained

Role of Magnetic Field for Instabilities in Relativistic Jets Yosuke Mizuno Institute for Theoretical Physics Goethe

Upper panel: the XRT light curve (0.3-10 keV) is shown with open black circles. Count rate-to-flux conversion factors were derived from time-dependent ...

Figure 2.

The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

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week11b p - UNLV Department of Physics and Astronomy .

Figure 7.

Warm Absorbers: Are They Disk Outflows? Daniel Proga UNLV.

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Ch 4 slides - UNLV Department of Physics and Astronomy

Collective molecular rotation in D2O - UNLV Department of Physics .

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Figure 1.

Figure 1.

Astronomy Astrophysics - UNLV Department of Physics and .

Magnetic Field Amplification by Turbulence in A Relativistic Shock Propagating through An Inhomogeneous Medium Yosuke Mizuno

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newsobserver.com AP Exclusive: China accuses outspoken tycoon in US of rape

The afterglow and host galaxy of GRB 090205 - UNLV Department .

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01_Introduction (Jan 18) - UNLV Department of Physics and .

3 Astrophysical ...

The CD Kink Instability in Magnetically Dominated Relativistic Jets * The relativistic jets associated with blazar

Figure 1.

The Formation and Structure of Stars

Relativistic MHD Simulations of Relativistic Jets with RAISHIN * We have developed a new three-

001 AST104(pdf) - UNLV Department of Physics .

Image: The 305-metre Arecibo telescope, in Puerto Rico, and its suspended support platform of radio receivers is shown amid a starry night.

Module on Computational Astrophysics Professor Jim Stone Department of Astrophysical Sciences and PACM.

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GRB 090926A and Bright Late-time Fermi Large Area - UNLV .

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Current-Driven Kink Instability in Magnetically Dominated Relativistic Jets Yosuke Mizuno Institute of Astronomy National

002 AST103 - UNLV Physics - University of .

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Figure 4.

Figure 1.

The red rows show the analogy with the supernova classification scheme. Blue cells show the properties of GRB 060614 (refs 7, 8, 9, 10).

GRB Afterglow Spectra Daniel Perley Astro 250 19 September* 2005 * International Talk Like a

2 Quasars * unsolved ...

Figure 6.

8 T +  Distributions 3 main ...

untitled 2 - UNLV Department of Physics and Astronomy - University .

Public Release of a Queryable Database of Galaxies in the Milennium Simulation

Figure 3.

AST 104 Introductory Astronomy: Stars and Galaxies - UNLV .

Astronomy Astrophysics - UNLV Department of Physics and Astronomy

Daniel Gumbiner

grb 110709a, 111117a, and 120107a - UNLV Department of .

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Figure 1.

002, Spring 2011 - UNLV Department of Physics and .

Figure 4.

The afterglow and host galaxy of GRB 090205 - UNLV Department .

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Figure 10.

Figure 2.

Panel (a)-(d): Light curves of GRB 060614 in different

Galileo wasn't the first to the Moon

Figure 1.

Figure 1.

Figure 3.

Background subtracted XRT light curve of GRB 050822 in the 0.3-10 keV energy band

Figure 1.

Figure 3.

Survey of the Universe Tom Burbine

3D GRMHD code: RAISHIN Yosuke Mizuno Institute for Theoretical Physics

Figure 3.

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Levels of organization: Stellar Systems Stellar Clusters Galaxies Galaxy Clusters Galaxy Superclusters The Universe Everyone

Plasmas in the Universe

002, Spring 2011 - UNLV Department of Physics and .

Evolution of the jet break time as a function of the redshift for three values of

The Evolution of AGN in Groups and Clusters - IPMU