144 Hypernovae PPTs View free & download

Magnetardriven Hypernovae PowerPoint PPT Presentation

Magnetardriven Hypernovae - Ideal Relativistic MHD - no physical resistivity (only numerical); 8. MFoGRBP, SAO, Bukovo ... 1) MHD waves must be able to escape from the black hole ergosphere ...

Ideal Relativistic MHD - no physical resistivity (only numerical); 8. MFoGRBP, SAO, Bukovo ... 1) MHD waves must be able to escape from the black hole ergosphere ...

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Gamma-ray bursts and hypernovae PowerPoint PPT Presentation

Gamma-ray bursts and hypernovae - GRB as superstrong cosmic explosions. Association with supernovae a critical view ... HETE2: GRB-X-ray rich-XRF (Lamb et al. 2003) Apparently continuous. transition ...

GRB as superstrong cosmic explosions. Association with supernovae a critical view ... HETE2: GRB-X-ray rich-XRF (Lamb et al. 2003) Apparently continuous. transition ...

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Hypernovae at the edge of the universe PowerPoint PPT Presentation

Hypernovae at the edge of the universe - Form of light: all light travels in waves classified according to ... Keck, Hawaii, 2days after outburst. Two months later - only a very faint galaxy remains ...

Form of light: all light travels in waves classified according to ... Keck, Hawaii, 2days after outburst. Two months later - only a very faint galaxy remains ...

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Neutron Stars PowerPoint PPT Presentation

Neutron Stars - Neutron Stars. Physics of ultradense, cold matter. Superfluidity, ... Origin of Spin, Kicks, B-field -- Magnetars vs. Pulsars. Hypernovae GRBs. Black Hole? ...

Neutron Stars. Physics of ultradense, cold matter. Superfluidity, ... Origin of Spin, Kicks, B-field -- Magnetars vs. Pulsars. Hypernovae GRBs. Black Hole? ...

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Diffusion of UltraHigh Energy Particles in Expanding Universe PowerPoint PPT Presentation

Diffusion of UltraHigh Energy Particles in Expanding Universe - sources of UHECR are unknown: are they galactic or extragalactic (AGN, GRB, Hypernovae... The only information comes from observations of Faraday rotation ...

sources of UHECR are unknown: are they galactic or extragalactic (AGN, GRB, Hypernovae... The only information comes from observations of Faraday rotation ...

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Gamma-ray Bursts and Particle Acceleration PowerPoint PPT Presentation

Gamma-ray Bursts and Particle Acceleration - To catch the sign of proton acceleration. GLAST will be Launched May in this year. ... Proton acceleration efficiency. We need 6-8 1043 ergs/Mpc3/yr to explain UHECRs ...

To catch the sign of proton acceleration. GLAST will be Launched May in this year. ... Proton acceleration efficiency. We need 6-8 1043 ergs/Mpc3/yr to explain UHECRs ...

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Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L PowerPoint PPT Presentation

Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L - Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L cher 08.12.2004 AK Astronomie Universit t Stuttgart Andreas M ller Theoriegruppe Landessternwarte ...

Gefangen im Wirbel aus Raum und Zeit - Rotierende Schwarze L cher 08.12.2004 AK Astronomie Universit t Stuttgart Andreas M ller Theoriegruppe Landessternwarte ...

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Exploding stars PowerPoint PPT Presentation

Exploding stars - Exploding stars And the modeling of Dwarf galaxies http://www.spacetoday.org/images/DeepSpace/Stars/StarWR124Hubble.jpg Dwarf Galaxies What are they?

Exploding stars And the modeling of Dwarf galaxies http://www.spacetoday.org/images/DeepSpace/Stars/StarWR124Hubble.jpg Dwarf Galaxies What are they?

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???? ??????? D3 PowerPoint PPT Presentation

???? ??????? D3 - d3 dc1 resceu ipmu ...

d3 dc1 resceu ipmu ...

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Gamma Ray Bursts PowerPoint PPT Presentation

Gamma Ray Bursts - Gamma Ray Bursts Shamelessly stolen from Chris Fryer s summer school lectures

Gamma Ray Bursts Shamelessly stolen from Chris Fryer s summer school lectures

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The MonKey Project PowerPoint PPT Presentation

The MonKey Project - The MonKey Project An Update on Stellar Yields

The MonKey Project An Update on Stellar Yields

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Agnieszka Janiuk PowerPoint PPT Presentation

Agnieszka Janiuk - Gamma rays are believed to come from the internal shocks, produced in the ... Collimation (1o ? 20o)? Rates (about 3 10-5 per year per galaxy) ...

Gamma rays are believed to come from the internal shocks, produced in the ... Collimation (1o ? 20o)? Rates (about 3 10-5 per year per galaxy) ...

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Neutron Stars and Black Holes PowerPoint PPT Presentation

Neutron Stars and Black Holes - Lines shift back and forth across each other every 164 days due to jet precession 0 SS 433 is most likely a black hole! In 1963, a nuclear test ban treaty was signed ...

Lines shift back and forth across each other every 164 days due to jet precession 0 SS 433 is most likely a black hole! In 1963, a nuclear test ban treaty was signed ...

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Relativistic photon mediated shocks PowerPoint PPT Presentation

Relativistic photon mediated shocks - Baryon poor fireball (BPJ) ~300. slow wind. Bow shock: source of keV photons. r 1011 cm ... (b)=baryons, ( ) = pairs, (r) = radiation. Basic equations. How to ...

Baryon poor fireball (BPJ) ~300. slow wind. Bow shock: source of keV photons. r 1011 cm ... (b)=baryons, ( ) = pairs, (r) = radiation. Basic equations. How to ...

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Rotating magnetized neutron stars PowerPoint PPT Presentation

Rotating magnetized neutron stars - J. Garrett Jernigan. MIT. George R. Ricker (PI) Geoffrey Crew ... Gilbert Vedrenne. Jean-Francois Olive. Michel Boer. UChicago. Donald Q. Lamb. Carlo Graziani ...

J. Garrett Jernigan. MIT. George R. Ricker (PI) Geoffrey Crew ... Gilbert Vedrenne. Jean-Francois Olive. Michel Boer. UChicago. Donald Q. Lamb. Carlo Graziani ...

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Neutron Stars and Black Holes - 0 Chapter 14 Neutron Stars and Black Holes

0 Chapter 14 Neutron Stars and Black Holes

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Diffusion of UltraHigh Energy Particles in Expanding Universe - Title: PowerPoint Presentation Author: GAZ Last modified by: GAZ Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3) Other titles

Title: PowerPoint Presentation Author: GAZ Last modified by: GAZ Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3) Other titles

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SOLVED AND UNSOLVED MYSTERIES IN GAMMA-RAY BURSTS PowerPoint PPT Presentation

SOLVED AND UNSOLVED MYSTERIES IN GAMMA-RAY BURSTS - Isotropic gamma-ray energies range from 1051 to 1054 erg ... THREE INTERESTING GAMMA-RAY BURST/SUPERNOVA PARAMETERS. THE Epeak-Eisotropic energy RELATION ...

Isotropic gamma-ray energies range from 1051 to 1054 erg ... THREE INTERESTING GAMMA-RAY BURST/SUPERNOVA PARAMETERS. THE Epeak-Eisotropic energy RELATION ...

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a MOnitoring NEtwork of Telescopes Dr. Frederic V. Hessman Prof. Klaus Beuermann UniversittsSternwar PowerPoint PPT Presentation

a MOnitoring NEtwork of Telescopes Dr. Frederic V. Hessman Prof. Klaus Beuermann UniversittsSternwar - Formation & Evolution of Planets. Sun / Dynamo-driven ... schools in the Ruhr Valley as well as in Lower Saxony. Summer 2002. The Basic Idea of the Project ...

Formation & Evolution of Planets. Sun / Dynamo-driven ... schools in the Ruhr Valley as well as in Lower Saxony. Summer 2002. The Basic Idea of the Project ...

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High energy Astrophysics PowerPoint PPT Presentation

High energy Astrophysics - High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 11. Gamma-ray bursts

High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 11. Gamma-ray bursts

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a brief history of PowerPoint PPT Presentation

a brief history of - a brief history of andreas m ller theory group max camenzind lsw heidelberg http://www.lsw.uni-heidelberg.de/users/amueller student seminar mpia & lsw

a brief history of andreas m ller theory group max camenzind lsw heidelberg http://www.lsw.uni-heidelberg.de/users/amueller student seminar mpia & lsw

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GRB Engines: Past and Current Models PowerPoint PPT Presentation

GRB Engines: Past and Current Models - I) Black hole accretion disk models (compact binary merger, collapsar) ... Black Hole Accretion Disk Models. Collapsar (aka hypernova: ...

I) Black hole accretion disk models (compact binary merger, collapsar) ... Black Hole Accretion Disk Models. Collapsar (aka hypernova: ...

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GRB Gamma Ray Bursts An Ongoing Mystery, Evolving Quickly PowerPoint PPT Presentation

GRB Gamma Ray Bursts An Ongoing Mystery, Evolving Quickly - GRB Gamma Ray Bursts An Ongoing Mystery, Evolving Quickly John G. Learned University of Hawaii with s from many folks, Particularly Kevin Hurley and Guido ...

GRB Gamma Ray Bursts An Ongoing Mystery, Evolving Quickly John G. Learned University of Hawaii with s from many folks, Particularly Kevin Hurley and Guido ...

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The Greatest Explosions since the Big Bang: PowerPoint PPT Presentation

The Greatest Explosions since the Big Bang: - Mosaic II = 36'x36' ESO WFI = 34'x33' OmegaCam = 1ox1o. 75' Student seminar ... Only if observing close to the ecliptic. Generally not associated with a galaxy ...

Mosaic II = 36'x36' ESO WFI = 34'x33' OmegaCam = 1ox1o. 75' Student seminar ... Only if observing close to the ecliptic. Generally not associated with a galaxy ...

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Stellar evolutionBirth to Death PowerPoint PPT Presentation

Stellar evolutionBirth to Death - After three centuries of work, we have a reasonably complete picture for how ... Possible Stellar Contrail? Quark Stars? RX J1856.5-3754. Dr. Jeremy Drake ...

After three centuries of work, we have a reasonably complete picture for how ... Possible Stellar Contrail? Quark Stars? RX J1856.5-3754. Dr. Jeremy Drake ...

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High%20Resolution%20X-Ray/UV%20Spectroscopy%20of%20the%20Intergalactic%20Medium:%20Hunting%20and%20Modeling%20the%20Missing%20Baryons%20in%20the%20WHIM - High Resolution X-Ray/UV Spectroscopy of the Intergalactic Medium: Hunting and Modeling the Missing Baryons in the WHIM Fabrizio Nicastro (Harvard-Smithsonian Center ...

High Resolution X-Ray/UV Spectroscopy of the Intergalactic Medium: Hunting and Modeling the Missing Baryons in the WHIM Fabrizio Nicastro (Harvard-Smithsonian Center ...

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??????????????? ???FMOS??????????? PowerPoint PPT Presentation

??????????????? ???FMOS??????????? - Title: Author: Tomonori Totani Last modified by: Created Date: 3/19/2004 4:44:39 AM

Title: Author: Tomonori Totani Last modified by: Created Date: 3/19/2004 4:44:39 AM

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Toward Understanding the Central Engine of Long GRBs PowerPoint PPT Presentation

Toward Understanding the Central Engine of Long GRBs - of relativistic jet (BZ-process, Neutrino Heating), which we are ... Neutrino heating processes have been included in the collapsar model. ...

of relativistic jet (BZ-process, Neutrino Heating), which we are ... Neutrino heating processes have been included in the collapsar model. ...

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Gamma Ray Bursts - 2004: Swift / BAT / XRT / UVOT. Early afterglows. Detected first short GRB afterglow. http://heasarc.gsfc.nasa.gov/docs/swift/swift.html. GRB Types and Light Curves ...

2004: Swift / BAT / XRT / UVOT. Early afterglows. Detected first short GRB afterglow. http://heasarc.gsfc.nasa.gov/docs/swift/swift.html. GRB Types and Light Curves ...

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The ATIC Experiment and Beyond PowerPoint PPT Presentation

The ATIC Experiment and Beyond - Louisiana State University, Baton Rouge, LA, USA ... 1051 ergs in the blast wave. SN rate 2/century 2X1049ergs/yr. Blast wave must convert ~1% of its energy into ...

Louisiana State University, Baton Rouge, LA, USA ... 1051 ergs in the blast wave. SN rate 2/century 2X1049ergs/yr. Blast wave must convert ~1% of its energy into ...

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Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). - Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode

Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode

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New Problems for a New Century PowerPoint PPT Presentation

New Problems for a New Century - You may find it useful to consult observations in other parts of the ... Precession. Bardeen-Petterson effect. Cosmology. 2nd/resumed inflation or new dynamics ...

You may find it useful to consult observations in other parts of the ... Precession. Bardeen-Petterson effect. Cosmology. 2nd/resumed inflation or new dynamics ...

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Padova talk - Estimate of magnification in SN1997ff smaller than in Benitez et al 2002, Riess et al 2004. ... Gravitational lensing (de)magnification not a problem for high-z SNe ...

Estimate of magnification in SN1997ff smaller than in Benitez et al 2002, Riess et al 2004. ... Gravitational lensing (de)magnification not a problem for high-z SNe ...

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Gravitational wave astronomy PowerPoint PPT Presentation

Gravitational wave astronomy - Passing GW causes changes in the interferometer arm lengths. ... Of known pulsars Crab pulsar is most promising source, also possible pulsar in SN1987A remnant. ...

Passing GW causes changes in the interferometer arm lengths. ... Of known pulsars Crab pulsar is most promising source, also possible pulsar in SN1987A remnant. ...

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The all-sky distribution of 511 keV electron-positron annihilation emission PowerPoint PPT Presentation

The all-sky distribution of 511 keV electron-positron annihilation emission - The bulge emission is spherically symmetric and is centred on the galactic ... The bulge emission arises from a different source which has only a weak or no ...

The bulge emission is spherically symmetric and is centred on the galactic ... The bulge emission arises from a different source which has only a weak or no ...

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Wide Field Optical Surveys - Wide Field Optical Surveys

Wide Field Optical Surveys

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Endpoints of stellar evolution PowerPoint PPT Presentation

Endpoints of stellar evolution - There is another effect that extends SN light curves: Radioactive decay ! (Frank Timmes) ... Nucleosynthesis is a prime constraint for models. 48 ...

There is another effect that extends SN light curves: Radioactive decay ! (Frank Timmes) ... Nucleosynthesis is a prime constraint for models. 48 ...

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The role of stars in AGN PowerPoint PPT Presentation

The role of stars in AGN - Lecture 3 The role of stars in AGN Evidence for stars in the nuclear regions of type-2 AGN Photoionization models for starbursts Type IIn supernovae: variability

Lecture 3 The role of stars in AGN Evidence for stars in the nuclear regions of type-2 AGN Photoionization models for starbursts Type IIn supernovae: variability

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Minor Planet Search Using TOAST PowerPoint PPT Presentation

Minor Planet Search Using TOAST - A set search pattern was used during the month of July and observations ... along a line for a half hour and then the pattern was repeated, giving two ...

A set search pattern was used during the month of July and observations ... along a line for a half hour and then the pattern was repeated, giving two ...

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Formation of Primordial Protostars The Final Chapter PowerPoint PPT Presentation

Formation of Primordial Protostars The Final Chapter - Formation of Primordial Protostars. The Final Chapter. Naoki ... Collision Induced Emission. During collisions, a collision. pair acts as a super-molecule' ...

Formation of Primordial Protostars. The Final Chapter. Naoki ... Collision Induced Emission. During collisions, a collision. pair acts as a super-molecule' ...

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and the Art of Robotic Telescopes Frederic V' Rick Hessman Klaus Beuermann UniversittsSternwarte Geo PowerPoint PPT Presentation

and the Art of Robotic Telescopes Frederic V' Rick Hessman Klaus Beuermann UniversittsSternwarte Geo - Need Your Own (Robotic) Small Telescopes. Projects which require large amounts of ... Stellar Seismology. Winter 2002/2003. Texas-G ttingen Exoplanet Search ...

Need Your Own (Robotic) Small Telescopes. Projects which require large amounts of ... Stellar Seismology. Winter 2002/2003. Texas-G ttingen Exoplanet Search ...

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Measuring the equation of state with highredshift supernovae - Measuring the equation of state with highredshift supernovae

Measuring the equation of state with highredshift supernovae

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Data Analysis Techniques for PowerPoint PPT Presentation

Data Analysis Techniques for - Classes of pulsars: fmax = 1 kHz, t = 40 yr; fmax = 200 Hz, t = 1000 yr. Stochastic Background ... where rk is the SNR in subband k (normalised templates) ...

Classes of pulsars: fmax = 1 kHz, t = 40 yr; fmax = 200 Hz, t = 1000 yr. Stochastic Background ... where rk is the SNR in subband k (normalised templates) ...

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By Adric Riedel PowerPoint PPT Presentation

By Adric Riedel - The Orion Nebula is one of the most prominent. ... Were it not for the radiation of the O stars, the Orion Nebula would be invisible. ...

The Orion Nebula is one of the most prominent. ... Were it not for the radiation of the O stars, the Orion Nebula would be invisible. ...

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Computational Nuclear Astrophysics at the Exascale PowerPoint PPT Presentation

Computational Nuclear Astrophysics at the Exascale - ... will allow unprecedented, high-resolution, multidimensional, multiphysics ... Exascale computing would allow high-resolution 3-D Radiation-magnetohydrodynamic ...

... will allow unprecedented, high-resolution, multidimensional, multiphysics ... Exascale computing would allow high-resolution 3-D Radiation-magnetohydrodynamic ...

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The case for High energy neutrino astronomy PowerPoint PPT Presentation

The case for High energy neutrino astronomy - [Blandford 76; Lovelace 76] [Waxman 95, Vietri 95, Milgrom & Usov 95] ... Linda Smith (University College London), WIYN//NSF, NASA/ESA. Robert Gendler. M82 M81 ...

[Blandford 76; Lovelace 76] [Waxman 95, Vietri 95, Milgrom & Usov 95] ... Linda Smith (University College London), WIYN//NSF, NASA/ESA. Robert Gendler. M82 M81 ...

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Xray Spectra of Clusters of Galaxies - Xray Spectra of Clusters of Galaxies

Xray Spectra of Clusters of Galaxies

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Supernovae - Supernovae Lab 9 Let s go Supernova! Stars which are 8x massive than our Sun end their lives in a most spectacular way; they go supernova!

Supernovae Lab 9 Let s go Supernova! Stars which are 8x massive than our Sun end their lives in a most spectacular way; they go supernova!

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Massive Star Models for Gamma-Ray Bursts* PowerPoint PPT Presentation

Massive Star Models for Gamma-Ray Bursts* - Title: PowerPoint Presentation Last modified by: Stan Woosley Created Date: 10/29/2001 7:41:19 PM Document presentation format: Custom Other titles

Title: PowerPoint Presentation Last modified by: Stan Woosley Created Date: 10/29/2001 7:41:19 PM Document presentation format: Custom Other titles

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Aucun titre de diapositive PowerPoint PPT Presentation

Aucun titre de diapositive - Service d'Astrophysique,CEA, Institut d'Astrophysique de Paris. OUTLINE ... MAJORANA PARTICULE (particle = antiparticle) Positrons produced by different channels ...

Service d'Astrophysique,CEA, Institut d'Astrophysique de Paris. OUTLINE ... MAJORANA PARTICULE (particle = antiparticle) Positrons produced by different channels ...

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Neutron Stars and Black Holes - A inch cube of this material with would weigh more than 100 million tons. ... gradually causes much of the disk material to eventually spiral into the black hole. ...

A inch cube of this material with would weigh more than 100 million tons. ... gradually causes much of the disk material to eventually spiral into the black hole. ...

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Gamma-Ray Bursts and their optical counterparts PowerPoint PPT Presentation

Gamma-Ray Bursts and their optical counterparts - fireball external shock with ISM - afterglow emission ... Optical telescopes (afterglow localization, brightness, decay index): always ...

fireball external shock with ISM - afterglow emission ... Optical telescopes (afterglow localization, brightness, decay index): always ...

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Search for the gravity wave signature of GRB030329/SN2003dh PowerPoint PPT Presentation

Search for the gravity wave signature of GRB030329/SN2003dh - The GRB Coordinates Network (GCN) The third InterPlanetary Network (IPN3) ... Due to the sub-burst longitude and latitude and the geographical distribution of ...

The GRB Coordinates Network (GCN) The third InterPlanetary Network (IPN3) ... Due to the sub-burst longitude and latitude and the geographical distribution of ...

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Sources of gravitational waves for groundbased detectors PowerPoint PPT Presentation

Sources of gravitational waves for groundbased detectors - Free precession. Was thought to damp in 1yr (vortex pinning) ... 22, 1825 (2005): Observations say precession lasts 10yr, visible to galactic ...

Free precession. Was thought to damp in 1yr (vortex pinning) ... 22, 1825 (2005): Observations say precession lasts 10yr, visible to galactic ...

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Universets voldsomste eksplosjoner PowerPoint PPT Presentation

Universets voldsomste eksplosjoner - ... har g tt p HETE-2 i verdensrommet, kommer alarmer til norske amat rastronomer via e-post og SMS-meldinger p mobiltelefon.

... har g tt p HETE-2 i verdensrommet, kommer alarmer til norske amat rastronomer via e-post og SMS-meldinger p mobiltelefon.

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Signal from GammaRay Bursts PowerPoint PPT Presentation

Signal from GammaRay Bursts - The Auto Correlation Function. Wavelet analysis. Power Density Spectra. Interpreting ... Quantify intrinsic delay, the 'pulse paradigm' can hide the QG effect ! ...

The Auto Correlation Function. Wavelet analysis. Power Density Spectra. Interpreting ... Quantify intrinsic delay, the 'pulse paradigm' can hide the QG effect ! ...

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Hypernovae PowerPoint PPT Presentations