33 Sn1006 PPTs View free & download

Modeling the Radiation from the Supernova Remnant of SN1006 - Modeling the Radiation from the Supernova Remnant of SN1006

Modeling the Radiation from the Supernova Remnant of SN1006

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Space Monkeys and How to Destroy Them PowerPoint PPT Presentation

Space Monkeys and How to Destroy Them - Space Monkeys and the Threat to Spacetime. History of Anti-Space ... SN1006 (Winkler et al. 2003) Went off in AD 1006. G.326.6 14.6. D=2.2kpc. z=555pc. R=6.8kpc ...

Space Monkeys and the Threat to Spacetime. History of Anti-Space ... SN1006 (Winkler et al. 2003) Went off in AD 1006. G.326.6 14.6. D=2.2kpc. z=555pc. R=6.8kpc ...

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ALMA's Window on Molecular Emission: Small Ions to Complex Prebiotics PowerPoint PPT Presentation

ALMA's Window on Molecular Emission: Small Ions to Complex Prebiotics - 1000 year anniversary of SN1006 this week! Correlator technology: Huge ... 2003 showed the distribution of HCOOH (greyscale) at 7 cm was very similar to ...

1000 year anniversary of SN1006 this week! Correlator technology: Huge ... 2003 showed the distribution of HCOOH (greyscale) at 7 cm was very similar to ...

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GeV-TeV Gamma-ray Astronomy PowerPoint PPT Presentation

GeV-TeV Gamma-ray Astronomy - International Workshop on Extremely High Energy Cosmic Rays, March 22-23, 2001, Kashiwa GeV-TeV Gamma-ray Astronomy Masaki Mori ICRR, Univ. Tokyo

International Workshop on Extremely High Energy Cosmic Rays, March 22-23, 2001, Kashiwa GeV-TeV Gamma-ray Astronomy Masaki Mori ICRR, Univ. Tokyo

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Suzaku Observation of SN 1006: Is it the PowerPoint PPT Presentation

Suzaku Observation of SN 1006: Is it the - Hiroya Yamaguchi, Katsuji Koyama, Hiroshi Nakajima (Kyoto Univ. ... emission or blast-wave component, the abundance. becomes more high. Therefore the value should ...

Hiroya Yamaguchi, Katsuji Koyama, Hiroshi Nakajima (Kyoto Univ. ... emission or blast-wave component, the abundance. becomes more high. Therefore the value should ...

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CANGAROO-III PowerPoint PPT Presentation

CANGAROO-III - STE Lab, Nagoya University. National Astronomical Observatory of Japan ... Alt-azimuth mount. Camera: T1: 552ch (2.7 FOV) T2,T3,T4: 427ch (4 FOV) Electronics: ...

STE Lab, Nagoya University. National Astronomical Observatory of Japan ... Alt-azimuth mount. Camera: T1: 552ch (2.7 FOV) T2,T3,T4: 427ch (4 FOV) Electronics: ...

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Supernova Remnants as Cosmic Rays Accelerators PowerPoint PPT Presentation

Supernova Remnants as Cosmic Rays Accelerators - Institute for Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of ... dcr ~ 10-3 at 1012 - 1014 eV - anisotropy. rg ~ 1E/(Z 3 1015 eV) pc - Larmor radius ...

Institute for Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of ... dcr ~ 10-3 at 1012 - 1014 eV - anisotropy. rg ~ 1E/(Z 3 1015 eV) pc - Larmor radius ...

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Search for Synchrotron X-ray Dominated SNRs PowerPoint PPT Presentation

Search for Synchrotron X-ray Dominated SNRs - log nt (cm-3s) 10.4 (10.1 11.9) ... We searched for the radio and gamma-ray counterparts, however, no counterpart was found except for G28.6-0.1 ...

log nt (cm-3s) 10.4 (10.1 11.9) ... We searched for the radio and gamma-ray counterparts, however, no counterpart was found except for G28.6-0.1 ...

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Risultati sperimentali recenti nella astrofisica gamma (Una selezione) PowerPoint PPT Presentation

Risultati sperimentali recenti nella astrofisica gamma (Una selezione) - Risultati sperimentali recenti nella astrofisica gamma (Una selezione) 1) EGRET 2) La Crab 3) AGN : Mrk 421 , Mrk 501 4) GRB 5) Sorgenti non identificate

Risultati sperimentali recenti nella astrofisica gamma (Una selezione) 1) EGRET 2) La Crab 3) AGN : Mrk 421 , Mrk 501 4) GRB 5) Sorgenti non identificate

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Science Capabilities - Summary PowerPoint PPT Presentation

Science Capabilities - Summary - ... synchrotron nebula around the Crab pulsar (the small dot at ... Galactic arm structure What are between arms? Correlation with radio, X & hard ... arm ...

... synchrotron nebula around the Crab pulsar (the small dot at ... Galactic arm structure What are between arms? Correlation with radio, X & hard ... arm ...

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X-Raying%20the%20Hot%20Universe PowerPoint PPT Presentation

X-Raying%20the%20Hot%20Universe - X-Ray Studies of Nucleosynthesis and Abundances in Supernova Remnants John P. Hughes Rutgers University

X-Ray Studies of Nucleosynthesis and Abundances in Supernova Remnants John P. Hughes Rutgers University

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High Resolution X-ray Spectroscopy of SN 1006 PowerPoint PPT Presentation

High Resolution X-ray Spectroscopy of SN 1006 - High Resolution X-ray Spectroscopy of SN 1006 X-ray Diagnostics of Astrophysical ... distance 2.1 kpc (Ghavamian et al. 2002, Winkler et al. 2002) 30 arcmin diameter ...

High Resolution X-ray Spectroscopy of SN 1006 X-ray Diagnostics of Astrophysical ... distance 2.1 kpc (Ghavamian et al. 2002, Winkler et al. 2002) 30 arcmin diameter ...

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TeV Gamma-ray Astronomy and UHECR-1 PowerPoint PPT Presentation

TeV Gamma-ray Astronomy and UHECR-1 - EGRET. Date/Group. Type. Source. Catalog Name. C. no. 1997/Whipple. Blazar. 1ES2344 ... Only two in EGRET Catalog. July 22-23, 2004. Trevor Weekes Watson Fest ...

EGRET. Date/Group. Type. Source. Catalog Name. C. no. 1997/Whipple. Blazar. 1ES2344 ... Only two in EGRET Catalog. July 22-23, 2004. Trevor Weekes Watson Fest ...

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COSMIC RAYS - Introduction to Cosmic Rays and Cosmic Air Shower Experiments Cosmic rays-a long story C.T.R Wilson discovered in 1900 the continuous atmospheric ionization.

Introduction to Cosmic Rays and Cosmic Air Shower Experiments Cosmic rays-a long story C.T.R Wilson discovered in 1900 the continuous atmospheric ionization.

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ALMA's Window on Molecular Emission: Small Ions to Complex Prebiotics - ALMA's Window on Molecular Emission: Small Ions to Complex Prebiotics Al Wootten

ALMA's Window on Molecular Emission: Small Ions to Complex Prebiotics Al Wootten

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TeV Gamma-ray Astronomy and UHECR-1 - TeV Gamma-ray Astronomy and UHECR-1 Trevor C. Weekes, Whipple Observatory, Harvard-Smithsonian Center for Astrophysics Outline Relevance to UHECR s Atmospheric ...

TeV Gamma-ray Astronomy and UHECR-1 Trevor C. Weekes, Whipple Observatory, Harvard-Smithsonian Center for Astrophysics Outline Relevance to UHECR s Atmospheric ...

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Particle Acceleration in SNR PowerPoint PPT Presentation

Particle Acceleration in SNR - Feedback from accelerating cosmic rays. Field amplification of plasma. Efficient cosmic ray acceleration. Bd = 126 G. Kep = 10-4. ESN = 1.8 x1051 erg ...

Feedback from accelerating cosmic rays. Field amplification of plasma. Efficient cosmic ray acceleration. Bd = 126 G. Kep = 10-4. ESN = 1.8 x1051 erg ...

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Section on Supernova remnants and cosmic rays of the White Paper on the Status and Future of Ground-based Gamma-ray Astronomy PowerPoint PPT Presentation

Section on Supernova remnants and cosmic rays of the White Paper on the Status and Future of Ground-based Gamma-ray Astronomy - Section on Supernova remnants and cosmic rays of the White Paper on the Status and Future of Ground-based Gamma-ray Astronomy 2008arXiv0810.0673

Section on Supernova remnants and cosmic rays of the White Paper on the Status and Future of Ground-based Gamma-ray Astronomy 2008arXiv0810.0673

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The structure and evolution of stars PowerPoint PPT Presentation

The structure and evolution of stars - The structure and evolution of stars Lecture13: Supernovae - deaths of massive stars Complete notes available online: http://star.pst.qub.ac.uk/~sjs/teaching.html

The structure and evolution of stars Lecture13: Supernovae - deaths of massive stars Complete notes available online: http://star.pst.qub.ac.uk/~sjs/teaching.html

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The Theory of Supernova Remnants PowerPoint PPT Presentation

The Theory of Supernova Remnants - The Theory of Supernova Remnants Some comments on Supernova Remnants and the production of Cosmic Rays Don Ellison, North Carolina State University

The Theory of Supernova Remnants Some comments on Supernova Remnants and the production of Cosmic Rays Don Ellison, North Carolina State University

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Mario A. Riquelme, Anatoly Spitkovsky PowerPoint PPT Presentation

Mario A. Riquelme, Anatoly Spitkovsky - In 2004 A. Bell predicted that plasma waves can be amplified non-resonantly (RL, ... MHD studies (Bell 2004). Va,0/Vd,cr = 1/40, Vd,cr=c (dash-dotted) ...

In 2004 A. Bell predicted that plasma waves can be amplified non-resonantly (RL, ... MHD studies (Bell 2004). Va,0/Vd,cr = 1/40, Vd,cr=c (dash-dotted) ...

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MHD instability PowerPoint PPT Presentation

MHD instability - The same MHD instability may be driven by fast electrons in ... The MHD instability grows more slowly than the Weibel instability, ...

The same MHD instability may be driven by fast electrons in ... The MHD instability grows more slowly than the Weibel instability, ...

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High energy emission from supernova remnants and regions of star formation PowerPoint PPT Presentation

High energy emission from supernova remnants and regions of star formation - ... radio map of the nearby star LS 5039 obtained with VLBA and VLA in ... No WR or Of massive stars in the field, no X-ray binaries or black hole candidates ...

... radio map of the nearby star LS 5039 obtained with VLBA and VLA in ... No WR or Of massive stars in the field, no X-ray binaries or black hole candidates ...

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The structure and evolution of stars - The Crab nebula - optical (red) and X-ray (lilac) composite. Death of a massive star ... are observed mostly in the gas and dust rich arms of spiral galaxies. ...

The Crab nebula - optical (red) and X-ray (lilac) composite. Death of a massive star ... are observed mostly in the gas and dust rich arms of spiral galaxies. ...

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The Slow XRay Expansion of the Northwestern Rim of RX J0852.04622 PowerPoint PPT Presentation

The Slow XRay Expansion of the Northwestern Rim of RX J0852.04622 - Vela Jr. was the 2nd object, which showed 44Ti decay line, following the Cas A SNR. ... of the g-ray line at 1.157 MeV seems to have no relation to Vela Jr. ...

Vela Jr. was the 2nd object, which showed 44Ti decay line, following the Cas A SNR. ... of the g-ray line at 1.157 MeV seems to have no relation to Vela Jr. ...

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Lecture 11 Stellar Evolution PowerPoint PPT Presentation

Lecture 11 Stellar Evolution - I should present EVIDENCE to support this theory. Not much time see text for more details ... 1 cubic cm would weigh ~1 ton on Earth. Fate of 'High-Mass' Stars ...

I should present EVIDENCE to support this theory. Not much time see text for more details ... 1 cubic cm would weigh ~1 ton on Earth. Fate of 'High-Mass' Stars ...

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Astrophysics and Cosmology with TeV gamma-rays - Astrophysics and Cosmology with TeV gammarays

Astrophysics and Cosmology with TeV gammarays

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Measurements of CosmicRay Positrons PowerPoint PPT Presentation

Measurements of CosmicRay Positrons - Uses 22 rad.length EM calorimeter with a 0.75 interaction length C target. ... Caution: Leakage out the back of calorimeter can lead to pileup at lower energy. ...

Uses 22 rad.length EM calorimeter with a 0.75 interaction length C target. ... Caution: Leakage out the back of calorimeter can lead to pileup at lower energy. ...

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The complex EAS hybrid arrays in Tibet PowerPoint PPT Presentation

The complex EAS hybrid arrays in Tibet - (2) Light components around the knee energy region obtained by Tibet ASgamma experiment. ... Energy flux and spectrum of HE particles at AS cores (Tibet) ...

(2) Light components around the knee energy region obtained by Tibet ASgamma experiment. ... Energy flux and spectrum of HE particles at AS cores (Tibet) ...

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TeV Gamma Ray Sky - TeV Gamma Ray Sky

TeV Gamma Ray Sky

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ISAPP 2003 - Crab Nebula: example of a neutron star formed during a supernova explosion. ... include the disk (containing the spiral arms), the halo, and the nucleus or ...

Crab Nebula: example of a neutron star formed during a supernova explosion. ... include the disk (containing the spiral arms), the halo, and the nucleus or ...

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Groundbased GammaRay Astronomy PowerPoint PPT Presentation

Groundbased GammaRay Astronomy - Several arrays of ground-based detectors achieve a sensitivity 1/100 of the flux ... view ~ 1 steradian) MILAGRO (LosAlamos, USA), Tibet ARGO (Yang Ba Jing, Tibet) ...

Several arrays of ground-based detectors achieve a sensitivity 1/100 of the flux ... view ~ 1 steradian) MILAGRO (LosAlamos, USA), Tibet ARGO (Yang Ba Jing, Tibet) ...

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A1257787023zJTme PowerPoint PPT Presentation

A1257787023zJTme - Rankine-Hugoniot jump conditions: postshock temperature mean ... SN 1993J (Fransson, Lundqvist & Chevalier 1996; not shown) Diagnostics at The Forward Shock of ...

Rankine-Hugoniot jump conditions: postshock temperature mean ... SN 1993J (Fransson, Lundqvist & Chevalier 1996; not shown) Diagnostics at The Forward Shock of ...

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Sn1006 PowerPoint PPT Presentations