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from H to Si and eventually explodes as a core collapse supernova. Mup' MPISN Massive stars ... Mass Loss (determine which stars explode as RSG and which as BSG) ...
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presupernova and then exploded. with pistons near the edge of the. iron core (S/NAk = 4.0) Each model exploded with a. variety of energies from 0.3 to. 10 x 1051 ...
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log LX (ergs/s) log Lopt (ergs/s) Age (yr) SN 1987A (PS) 33.74 33.9 16.75 ... Constructing of evolutionary presupernova models (1964 1987) Main issues of SN 1987 A ...
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It comes from an era soon after stars and galaxies first formed, about 500 ... core collapses in a self similar fashion. Were G = 4/3 for the entire iron ...
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Semiconvection is the term applied to the slow mixing that goes ... Altair ( Aquilae) veq ' 230 km/sec. Teff4 / geff * tKH. Effects of rotation ...
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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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NUCLEOSYNTHESIS IN STELLAR EVOLUTION AND EXPLOSIONS: ABUNDANCE YIELDS FOR CHEMICAL EVOLUTION. ... Jaeger et al. (2001): 22Ne(a,n)25Mg. Kunz et al. (2001): 12C(a,g)16O ...
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of Z = 0 Stars, 12 100. The evolution of Z = 0 massive stars has been studied for. many years, e.g. Ezer & Cameron ... Use Kepler implicit hydrodynamics code ...
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Stability of compact stars (white dwarfs and neutron stars) . G.S.Bisnovatyi-Kogan Space Research Institute RAN, Moscow Joint Institute of Nuclear Researches, Dubna
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Observed properties of SN. From Woosley Lecture 16. See also Filippenko (1997; ... Lack hydrogen, but also lack the Si II ll6355 feature that typifies. SN Ia. ...
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Title: Magnetorotational mechanism: 2D Simulations of Supernova Explosions and ejections Author: max Last modified by: GENA Created Date: 2/5/2001 1:31:21 PM
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Problems of cosmogony (1963), 9, 254-262 (in Russian) ... Ya.B. Zeldovich, Problems of cosmogony (1963), 9, 157-175 (in Russian) ...
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... beam, a shocked cocoon, and a bow shock, and it is narrowly collimated ... with a cocoon surrounding the jet beam and a dense 'plug' at the head of the jet ...
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Generic picture of an accreting system (pm,swift) A collapse of a rotating envelope ... Timing is good as SWIFT is to be launched soon. It used to be used ...
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Title: Slide 1 Author: Stan Woosley Last modified by: Stan Woosley Created Date: 3/17/2002 12:16:55 AM Document presentation format: On-screen Show
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evidence for a mild association with spiral arms ... Found in spiral arms and. star forming regions. Not found in ellipticals. ... 1 SNu == one supernova per century ...
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Core-Collapse Supernovae: Magnetorotational Explosions and Jet ... MERLIN 5GHz. Fender (1999) X-ray image of. microquasar. XTE J1550-564(center) with two jets. ...
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Barge, LAM Rauer Bouchy. Moutou, LAM. Deeg, ? Rouan, IDF group. Ollivier IDF Team. Rauer, german team Deleuil, Barge. Queloz, Geneve team - Follow-up: ...
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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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It indicates GRB is collimated outflow. Jet angle ~a few degrees ... Magnetic field is helpful to collimate the jet. Observation (although controversial) ...
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http://www.supernovae.net/snimages/snlinks.html#Catalogs ... 1200 2000 Angstrom band). The ionization threshold for these. species is 30 to 80 keV. ...
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Depending on T the different branchings become active. In all cases the result is ... Balance between forward and reverse reactions for increasing number of processes ...
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Because of the general tendency of the interior temperature of ... For radiative opacities other than kes, in particular kbf and kbb, ...
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Missing fundamental physics (still discussed) BBAL 1979. The explosion was low entropy ... Tough physics nuclear EOS, neutrino opacities ...
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Supernova Grand Challenges on ATLAS R. D. Hoffman Nuclear Theory & Modeling Group N-DIV - LLNL This work performed under the auspices of the U.S. Department of Energy by
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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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Optimization of codes on parallel computers. Manipulation. and visualization of large data sets. ... particle based code (SPH) and rudimentary neutrino ...
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Fundamental nuclear physics properties of the atomic nucleus, ... 3. Physics of hydrogen burning in massive stars, the CNO-tri-cycle, ...
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compact blue giants depending ... Eta Car. 136-155 M. Massey & Hunter (1998) R136a1. Bonanos et al. (2004) ... Eta Car. Calculations suggested that strong ...
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Late F stars also show Li depletion due to coupled rotational/wave mixing at ... M , tip of RGB at fixed luminosity (for given z) so acts as standard-ish candle. ...
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Constraint on OSC parameters from the detection of supernova neutrino burst ... time neutrino burst model available ... Analysis by using the TBP burst model ...
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It is analogous, in ways, to neon burning in that it ... i.e., the energy required to dissociate the nucleus AZ into. 28Si and particles. ...
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A historical split in the way convection is treated in a stellar ... condition can be written two ways one ... Goldreich-Schubert-Fricke. Solberg Hoiland ...
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