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H.Nomoto PowerPoint PPT Presentation
H.Nomoto - Set delay parameters to ASICs on PS boards ... Set coarse delay parameters in PP ASICs to the values calculated from cable length ...
Set delay parameters to ASICs on PS boards ... Set coarse delay parameters in PP ASICs to the values calculated from cable length ...
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Ay123 Lecture I - Physical Properties PowerPoint PPT Presentation
Ay123 Lecture I - Physical Properties - ... C-O WD systems (Nomoto et al astro-ph/9907386) WD red giant ... WD MS in common envelope. AGB with C O core. RG He core. Significant time delay ...
... C-O WD systems (Nomoto et al astro-ph/9907386) WD red giant ... WD MS in common envelope. AGB with C O core. RG He core. Significant time delay ...
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Progress in radiative transfer modelling PowerPoint PPT Presentation
Progress in radiative transfer modelling - Progress in. radiative transfer modelling. First International ... averaged chemical composition above the photosphere (Nomoto et al., 1984, ApJ. 286, 644) ...
Progress in. radiative transfer modelling. First International ... averaged chemical composition above the photosphere (Nomoto et al., 1984, ApJ. 286, 644) ...
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H'Nomoto PowerPoint PPT Presentation
H'Nomoto - Solenoid and barrel toroid magnets were installed. ... Parts checked in sector test. Full big wheels. test in the pit. 27. PP. delay. BCID. SLB ASIC ...
Solenoid and barrel toroid magnets were installed. ... Parts checked in sector test. Full big wheels. test in the pit. 27. PP. delay. BCID. SLB ASIC ...
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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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EXPLOSION OF VERY MASSIVE STARS AND THE ORIGIN OF INTERMEDIATE MASS BLACK HOLES PowerPoint PPT Presentation
EXPLOSION OF VERY MASSIVE STARS AND THE ORIGIN OF INTERMEDIATE MASS BLACK HOLES - I. INTRODUCTION. II. OUR RECENT RESEARCH. III. SUMMARY/CONCLUSION. 3 ... consistent with IMBH mass (iii) Abundance pattern ...consistent with M82 gas, ICM, IGM ...
I. INTRODUCTION. II. OUR RECENT RESEARCH. III. SUMMARY/CONCLUSION. 3 ... consistent with IMBH mass (iii) Abundance pattern ...consistent with M82 gas, ICM, IGM ...
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White dwarf mergers PowerPoint PPT Presentation
White dwarf mergers - The British Council, JSPS, PPARC. based on work published in MNRAS ... (Landau & Lifshitz 1958) CO He merger frequency: 4.4 10-3 yr-1 (Neleman's et al. 2001) ...
The British Council, JSPS, PPARC. based on work published in MNRAS ... (Landau & Lifshitz 1958) CO He merger frequency: 4.4 10-3 yr-1 (Neleman's et al. 2001) ...
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The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars PowerPoint PPT Presentation
The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars - 24, June 2002. white dwarf mergers. The progeny of binary white dwarf mergers; ... Progeny of WD WD mergers ? Extreme Helium stars. RCrB stars. subdwarf B stars ...
24, June 2002. white dwarf mergers. The progeny of binary white dwarf mergers; ... Progeny of WD WD mergers ? Extreme Helium stars. RCrB stars. subdwarf B stars ...
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Nucleosynthesis in metalfree and metalpoor stars PowerPoint PPT Presentation
Nucleosynthesis in metalfree and metalpoor stars - (C from He burning. mixed into H burning. shell CN cycle), also sources for C, O ... Hydrostatic and explosive burning. From C to the Fe group ...
(C from He burning. mixed into H burning. shell CN cycle), also sources for C, O ... Hydrostatic and explosive burning. From C to the Fe group ...
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TMT Observational study of nearby supernovae with TMT and smaller telescopes PowerPoint PPT Presentation
TMT Observational study of nearby supernovae with TMT and smaller telescopes - SN 2006gy: One of the most luminous SNe. MV ~ -22 mag? Lbol~3 1044 erg s-1; slow LC evolution, ... Likely more luminous than SN 2006gz (56Ni mass 1.2 M ...
SN 2006gy: One of the most luminous SNe. MV ~ -22 mag? Lbol~3 1044 erg s-1; slow LC evolution, ... Likely more luminous than SN 2006gz (56Ni mass 1.2 M ...
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NeXT???? ??????????? PowerPoint PPT Presentation
NeXT???? ??????????? - NeXT ...
NeXT ...
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The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars PowerPoint PPT Presentation
The progeny of binary white dwarf mergers extreme helium stars, R CrB stars and subdwarf B stars - white dwarf mergers. The progeny of binary white dwarf mergers; ... (Landau & Lifshitz 1958) CO He merger frequency: 4.4 10-3 yr-1 (Neleman's et al. 2001) ...
white dwarf mergers. The progeny of binary white dwarf mergers; ... (Landau & Lifshitz 1958) CO He merger frequency: 4.4 10-3 yr-1 (Neleman's et al. 2001) ...
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SSP vs Galaxies PowerPoint PPT Presentation
SSP vs Galaxies - First consistent chemo stellar evolution spectral code by Bressan et al 94. Many ... PAH model (Li & Draine 01, Vega et al 05) needs revison above 14 mm ...
First consistent chemo stellar evolution spectral code by Bressan et al 94. Many ... PAH model (Li & Draine 01, Vega et al 05) needs revison above 14 mm ...
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Collaborators: PowerPoint PPT Presentation
Collaborators: - Gordon Garmire (Penn State) A Candidate Neutron Star & Its Association with Sgr A East ... Mach number ~ 2.2: v ~ 880 km s-1. for ISM kT ~ 1 keV ...
Gordon Garmire (Penn State) A Candidate Neutron Star & Its Association with Sgr A East ... Mach number ~ 2.2: v ~ 880 km s-1. for ISM kT ~ 1 keV ...
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TMR4220 Lecture PowerPoint PPT Presentation
TMR4220 Lecture - Linear equations of motion. Characteristic equations for stability analysis ... International Towing Tank Conference (ITTC) and Society of Naval Architects and ...
Linear equations of motion. Characteristic equations for stability analysis ... International Towing Tank Conference (ITTC) and Society of Naval Architects and ...
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The endpoint of massive stars in binaries: singlets, doublets? Triplets! PowerPoint PPT Presentation
The endpoint of massive stars in binaries: singlets, doublets? Triplets! - The endpoint of massive stars in binaries: singlets, doublets? ... Baryon poor outflows. GRB. 3e50erg. Black hole output. Rotational energy of black hole ...
The endpoint of massive stars in binaries: singlets, doublets? ... Baryon poor outflows. GRB. 3e50erg. Black hole output. Rotational energy of black hole ...
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Thermonuclear Supernova: A Successful Failure PowerPoint PPT Presentation
Thermonuclear Supernova: A Successful Failure - ASC Alliances Center for Thermonuclear Flashes, University of Chicago ... Foreplay counts: forgotten tale of the ICs. Confronting DFD with observations. Summary ...
ASC Alliances Center for Thermonuclear Flashes, University of Chicago ... Foreplay counts: forgotten tale of the ICs. Confronting DFD with observations. Summary ...
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Design Study of Fusion DEMO Plant at JAERI PowerPoint PPT Presentation
Design Study of Fusion DEMO Plant at JAERI - Design Study of Fusion DEMO Plant. at JAERI. Japan Atomic Energy Research Institute ... Yet, the reactor weight is still light compared with other tokamak designs. ...
Design Study of Fusion DEMO Plant. at JAERI. Japan Atomic Energy Research Institute ... Yet, the reactor weight is still light compared with other tokamak designs. ...
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Supernova and GRB remnants and their GeVTeV gray emission PowerPoint PPT Presentation
Supernova and GRB remnants and their GeVTeV gray emission - TeV unidentified (TeV unID) sources. No counterpart, Origin unknown ... isotropic ~200 keV, nonthermal. 10-3s~103s : Short, Long. GRB. Afterglow. X. Opt. Radio ...
TeV unidentified (TeV unID) sources. No counterpart, Origin unknown ... isotropic ~200 keV, nonthermal. 10-3s~103s : Short, Long. GRB. Afterglow. X. Opt. Radio ...
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Model Chemical Evolution: PowerPoint PPT Presentation
Model Chemical Evolution: - Model Chemical Evolution: Starburst Environment. Once upon a time... Starburst environment, chemical evolution plays an important role. ...
Model Chemical Evolution: Starburst Environment. Once upon a time... Starburst environment, chemical evolution plays an important role. ...
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Kick velocity PowerPoint PPT Presentation
Kick velocity - Kick velocity Why do neutron stars move so rapidly? Stars vs. Neutron Stars Pulsar velocity distribution SN explosions should not be symmetric! SN and kick explosion ...
Kick velocity Why do neutron stars move so rapidly? Stars vs. Neutron Stars Pulsar velocity distribution SN explosions should not be symmetric! SN and kick explosion ...
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Duchenne Muscular Dystrophy PowerPoint PPT Presentation
Duchenne Muscular Dystrophy - Duchenne Muscular Dystrophy Curtis Kendall December 5, 2006 Duchenne Muscular Dystrophy Facts DMD affects mostly males at a rate of 1 in 3,500 births.
Duchenne Muscular Dystrophy Curtis Kendall December 5, 2006 Duchenne Muscular Dystrophy Facts DMD affects mostly males at a rate of 1 in 3,500 births.
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Diapositive 1 PowerPoint PPT Presentation
Diapositive 1 - Wolf-Rayet Stars ... become Wolf-Rayet star is decreased for higher rotation ... A STRIKING OBSERVATIONAL FACTS. Very Helium-rich stars in Centuri ? DY/DZ ...
Wolf-Rayet Stars ... become Wolf-Rayet star is decreased for higher rotation ... A STRIKING OBSERVATIONAL FACTS. Very Helium-rich stars in Centuri ? DY/DZ ...
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Prospects of supernova neutrino observation by large detectors PowerPoint PPT Presentation
Prospects of supernova neutrino observation by large detectors - Use SN data to learn about particle physics properties of neutrinos ... Requires megaton detector Gd. 100% neutron tag assumed, Kachelriess et al 04 ...
Use SN data to learn about particle physics properties of neutrinos ... Requires megaton detector Gd. 100% neutron tag assumed, Kachelriess et al 04 ...
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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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Thermonuckear Supernovae: Stellar Explosions in Three Dimensions PowerPoint PPT Presentation
Thermonuckear Supernovae: Stellar Explosions in Three Dimensions - ASC Alliances Center for Thermonuclear Flashes, University of Chicago ... 3-D deflagration models (NRL, MPA, Barcelona, Chicago) 3-D DDT models (NRL) ...
ASC Alliances Center for Thermonuclear Flashes, University of Chicago ... 3-D deflagration models (NRL, MPA, Barcelona, Chicago) 3-D DDT models (NRL) ...
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Organic Electronics PowerPoint PPT Presentation
Organic Electronics - L. Ficke,M. Cahay, 'The bright future of organic LEDs', IEEE ... Broad color gamut. Wide viewing angle (~180 ) Good contrast. High resolution ( 5 m pixel size) ...
L. Ficke,M. Cahay, 'The bright future of organic LEDs', IEEE ... Broad color gamut. Wide viewing angle (~180 ) Good contrast. High resolution ( 5 m pixel size) ...
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Upalni biljezi u akutnom koronarnom sindromu PowerPoint PPT Presentation
Upalni biljezi u akutnom koronarnom sindromu - Upalni biljezi u akutnom koronarnom sindromu M. Bergovec, Z. Trstenjak, V. Raos, S. Pavlovi , M. Ragu , J. iki Vagi , . Romi , D. Kranj ec
Upalni biljezi u akutnom koronarnom sindromu M. Bergovec, Z. Trstenjak, V. Raos, S. Pavlovi , M. Ragu , J. iki Vagi , . Romi , D. Kranj ec
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Probing structure formation PowerPoint PPT Presentation
Probing structure formation - Probing structure formation & evolution with galaxy groups Jesper Rasmussen (Univ. of Birmingham) Main collaborators: T. Ponman S. Raychadhury T. Miles
Probing structure formation & evolution with galaxy groups Jesper Rasmussen (Univ. of Birmingham) Main collaborators: T. Ponman S. Raychadhury T. Miles
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Which Stars form Neutron Stars and Black Holes? PowerPoint PPT Presentation
Which Stars form Neutron Stars and Black Holes? - Which Stars form Neutron Stars and Black Holes
Which Stars form Neutron Stars and Black Holes
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Automobile Lane Detection System-on-Chip Integrated with Mixed Signal Mode CMOS Image Sensor PowerPoint PPT Presentation
Automobile Lane Detection System-on-Chip Integrated with Mixed Signal Mode CMOS Image Sensor - Yang and G. Jianhong, A 256x256 Pixel Smart CMOS Image Sensor ... Coulombe, J., Sawan, M. and Wang, C., Variable Resolution CMOS Current Mode Active Sensor ...
Yang and G. Jianhong, A 256x256 Pixel Smart CMOS Image Sensor ... Coulombe, J., Sawan, M. and Wang, C., Variable Resolution CMOS Current Mode Active Sensor ...
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Supernovae PowerPoint PPT Presentation
Supernovae - Type Ia supernovae are the biggest. thermonuclear explosions in ... This is the smallest length scale that can be deformed. by turbulence before burning first. ...
Type Ia supernovae are the biggest. thermonuclear explosions in ... This is the smallest length scale that can be deformed. by turbulence before burning first. ...
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Translation Initiation from the Ribosomal A Site or the P Site, Dependent on the conformation of RNA PowerPoint PPT Presentation
Translation Initiation from the Ribosomal A Site or the P Site, Dependent on the conformation of RNA - Elongation: Subsequent amino acids are attached to the growing polypeptide chain ... Elongation factors (EF-Tu, EF-Ts and ... Elongation, cont. ( Translocation) ...
Elongation: Subsequent amino acids are attached to the growing polypeptide chain ... Elongation factors (EF-Tu, EF-Ts and ... Elongation, cont. ( Translocation) ...
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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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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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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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The star formation history and the N/O abundance Mercedes Moll PowerPoint PPT Presentation
The star formation history and the N/O abundance Mercedes Moll - ... is dominated mainly by the third dredge up events and the Hot Bottom Burning processes ... increases allowing for more dredge-up events to occur, increasing ...
... is dominated mainly by the third dredge up events and the Hot Bottom Burning processes ... increases allowing for more dredge-up events to occur, increasing ...
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Aditya P. Mathur PowerPoint PPT Presentation
Aditya P. Mathur - Microsoft quality gate criteria. Pioneered by Praerit Garg [MS'95] ... Levy K.L.; Kipke D.R. A computational model of the cochlear nucleus octopus cell. ...
Microsoft quality gate criteria. Pioneered by Praerit Garg [MS'95] ... Levy K.L.; Kipke D.R. A computational model of the cochlear nucleus octopus cell. ...
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The oxygen abundance of HE 13272326 PowerPoint PPT Presentation
The oxygen abundance of HE 13272326 - Sean Ryan. Aaron Steinhauer. Masahide Takeda-Hidai. Stelios Tsangarides. Yuzuru Yoshii ... Paul Barklem. Timothy Beers. Kjell Eriksson. Constantine Delyannis ...
Sean Ryan. Aaron Steinhauer. Masahide Takeda-Hidai. Stelios Tsangarides. Yuzuru Yoshii ... Paul Barklem. Timothy Beers. Kjell Eriksson. Constantine Delyannis ...
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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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Chemical Evolution of the Milky Way PowerPoint PPT Presentation
Chemical Evolution of the Milky Way - Mass to light ratios vs. Galaxy absolute V magnitude (Gilmore et al. 2006) ... Carigi, Hernandez & Gilmore (2002) computed models for 4 dSphs by assuming SF ...
Mass to light ratios vs. Galaxy absolute V magnitude (Gilmore et al. 2006) ... Carigi, Hernandez & Gilmore (2002) computed models for 4 dSphs by assuming SF ...
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White dwarf mergers and the progeny of helium stars PowerPoint PPT Presentation
White dwarf mergers and the progeny of helium stars - P.W.Hill, St Andrews University, V.Woolf, Armagh PPARC. based on work published in MNRAS 313, 671, MNRAS 321,111 and submitted to MNRAS ...
P.W.Hill, St Andrews University, V.Woolf, Armagh PPARC. based on work published in MNRAS 313, 671, MNRAS 321,111 and submitted to MNRAS ...
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TMR 4220 Naval Hydrodynamics Manoeuvring and Ship Handling PowerPoint PPT Presentation
TMR 4220 Naval Hydrodynamics Manoeuvring and Ship Handling - Track reach in the full astern stopping test should not exceed 15 ship lengths ... Full astern stopping test results in extreme termal loads on the engine ...
Track reach in the full astern stopping test should not exceed 15 ship lengths ... Full astern stopping test results in extreme termal loads on the engine ...
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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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Abundances in intragroup gas PowerPoint PPT Presentation
Abundances in intragroup gas - Fe mass in the central peak normalised to K band luminosity of central galaxy ... Galaxy groups, like cool core clusters, have central abundance peaks dominated ...
Fe mass in the central peak normalised to K band luminosity of central galaxy ... Galaxy groups, like cool core clusters, have central abundance peaks dominated ...
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Nessun titolo diapositiva PowerPoint PPT Presentation
Nessun titolo diapositiva - Nessun titolo diapositiva
Nessun titolo diapositiva
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Explosive Nucleosynthesis PowerPoint PPT Presentation
Explosive Nucleosynthesis - This material expands, then cools nearly adiabatically ... Mole. Number. Neutron-rich. 1. Entropy. Radius. The disk responsible. for rapidly feeding a ...
This material expands, then cools nearly adiabatically ... Mole. Number. Neutron-rich. 1. Entropy. Radius. The disk responsible. for rapidly feeding a ...
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What Are Type Ia Supernovae? PowerPoint PPT Presentation
What Are Type Ia Supernovae? - Accretion from a binary companion leads to growth of the WD to the critical Chandrasekhar mass ... even unbind a Chandrasekhar mass WD... Jens C. Niemeyer ...
Accretion from a binary companion leads to growth of the WD to the critical Chandrasekhar mass ... even unbind a Chandrasekhar mass WD... Jens C. Niemeyer ...
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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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The Evolution and Explosion PowerPoint PPT Presentation
The Evolution and Explosion - The origin of the elements is an interesting problem ... is something fascinating about. science. One gets ... of fact.' Mark Twain in Life on the Mississippi ...
The origin of the elements is an interesting problem ... is something fascinating about. science. One gets ... of fact.' Mark Twain in Life on the Mississippi ...
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PHYSICS POTENTIAL OF SUPERNOVA NEUTRINOS PowerPoint PPT Presentation
PHYSICS POTENTIAL OF SUPERNOVA NEUTRINOS - PHYSICS POTENTIAL. OF. SUPERNOVA NEUTRINOS. Alessandro MIRIZZI. Dip.to di ... D 65, 073008 ... neutron capture [J.F.Beacom, and M.R.Vagins, 'GADZOOKS! ...
PHYSICS POTENTIAL. OF. SUPERNOVA NEUTRINOS. Alessandro MIRIZZI. Dip.to di ... D 65, 073008 ... neutron capture [J.F.Beacom, and M.R.Vagins, 'GADZOOKS! ...
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White dwarf merger as origin for extreme helium stars PowerPoint PPT Presentation
White dwarf merger as origin for extreme helium stars - H.Saio, Tohoku University, Sendai, Japan ... D.Pollacco, Queens University Belfast, R.Starling, MSSL, P.W.Hill, St Andrews University, V.Woolf, Armagh PPARC ...
H.Saio, Tohoku University, Sendai, Japan ... D.Pollacco, Queens University Belfast, R.Starling, MSSL, P.W.Hill, St Andrews University, V.Woolf, Armagh PPARC ...
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Michael Zingale PowerPoint PPT Presentation
Michael Zingale - Michael Zingale
Michael Zingale
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GRB PowerPoint PPT Presentation
GRB - ... and are also thermalized to a high temperature. The clever part is next: consider what would happen if, as a result of its thermal motion, ... (D~3 Gpc) L ~ fD2 ...
... and are also thermalized to a high temperature. The clever part is next: consider what would happen if, as a result of its thermal motion, ... (D~3 Gpc) L ~ fD2 ...
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Hydrogen Burning Nucleosynthesis, PowerPoint PPT Presentation
Hydrogen Burning Nucleosynthesis, - How hot do they get? Shear mixing during accretion. Convective 'undershoot' during burst ... Fourteen consecutive flashes. The first is a start up transient. GS ...
How hot do they get? Shear mixing during accretion. Convective 'undershoot' during burst ... Fourteen consecutive flashes. The first is a start up transient. GS ...
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NeutrinoPowered Explosions PowerPoint PPT Presentation
NeutrinoPowered Explosions - Missing fundamental physics (still discussed) BBAL 1979. The explosion was low entropy ... Tough physics nuclear EOS, neutrino opacities ...
Missing fundamental physics (still discussed) BBAL 1979. The explosion was low entropy ... Tough physics nuclear EOS, neutrino opacities ...
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