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The disappearance of the progenitors of supernovae 1993J and

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Producing Runaway Stars

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sorbent using peptides Fragments of apolipoprotein B-100

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The anxiolytic and analgesic properties of fenobam, a potent

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MMT Hypervelocity Star Survey

km s−1 at 50 kpc and 260 km s−1 at 100 kpc (Fig- ure 3).Binary Star Properties Both the supernova and binary-binary ejection mech-

Enzymically mediated bioprecipitation of uranium by a

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Plasma mediated off-resonance plasmonic enhanced ultrafast

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A Successful 3D Core-Collapse Supernova Explosion Model

A Successful 3D Core-Collapse Supernova Explosion Model In this paper, we The model explodes within $\sim$100 milliseconds of bounce (near when the

of Gravitational Waves from Core-Collapse Supernovae

Abstract: Recent core-collapse supernova (CCSN) simulations have predicted (100-300 Hz) potentially induced by the standing accretion shock instability

for the Laboratory Simulation of Supernova Hydrodynamics

hose type (e.g., Schmidt, 1966), then a 1999 LABORATORY SIMULATION OF SUPERNOVA 100 km s~1 would have Ðnds again that the

Testing Feedback Models with Nearby Star Forming Regions

large numbers of spatially resolved massive stars at a pre-supernovae stage3-9, as a result of limiting simulations to an upper limit of 100 M

The formation of massive black holes through collision run

instead of the standard 100 M⊙ used in the 10 Supplementary material This part of the paper at the time of supernova is 22–36 percent

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Effect of plasminogen activator (urokinase), plasmin, and

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On VI, N V, and C IV in the Galactic Halo. II. Velocity-

1 12.96 1. 100 14.40 0.22 13.00 1 100 14.30 250c 14.50 200c(1990), and cooling supernova remnant shells ( pluses, Slavin Cox 1993

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Observations of TeV Gamma Rays from Supernova Remnants

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Solving the Cosmic Lithium Problems with Gravitino Dark

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Radio observations of the bright X-ray supernova remnant G156

Radio observations of the bright X-ray supernova remnant G156.2+5.7The Effelsberg 100-m telescope has been used to map this object at 1448

Time Dilation in Type Ia Supernova Spectra at High Redshift

(typically accurate to 100 km s−1; see Falco et al. 1999) yields aTABLE 1 Comparison of galaxy and supernova redshifts SN zGAL (1) (2)

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Watching a New Star Make the Universe Dusty

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