Search Results - "Paxton, Bill"

MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS by Choi, Jieun, Dotter, Aaron, Conroy, Charlie, Cantiello, Matteo, Paxton, Bill, Johnson, Benjamin D.

“…ABSTRACT This is the first of a series of papers presenting the Modules for Experiments in Stellar Astrophysics (MESA) Isochrones and Stellar Tracks (MIST)…”
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Inferring Explosion Properties from Type II-Plateau Supernova Light Curves by Goldberg, Jared A., Bildsten, Lars, Paxton, Bill

“…We present advances in modeling Type IIP supernovae (SNe IIP) using MESA for evolution to shock breakout coupled with STELLA for generating light and radial…”
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ANGULAR MOMENTUM TRANSPORT WITHIN EVOLVED LOW-MASS STARS by Cantiello, Matteo, MANKOVICH, CHRISTOPHER, Bildsten, Lars, Christensen-Dalsgaard, Jorgen, Paxton, Bill

“…Asteroseismology of 1.0-2.0 M sub([middot in circle]) red giants by the Kepler satellite has enabled the first definitive measurements of interior rotation in…”
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CARBON SHELL OR CORE IGNITIONS IN WHITE DWARFS ACCRETING FROM HELIUM STARS by Brooks, Jared, Bildsten, Lars, Schwab, Josiah, Paxton, Bill

“…ABSTRACT White dwarfs accreting from helium stars can stably burn at the accreted rate and avoid the challenge of mass loss associated with unstable helium…”
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Accretion-induced Collapse from Helium Star + White Dwarf Binaries by Brooks, Jared, Schwab, Josiah, Bildsten, Lars, Quataert, Eliot, Paxton, Bill

“…Accretion-induced collapse (AIC) occurs when an O/Ne white dwarf (WD) grows to nearly the Chandrasekhar mass ( ), reaching central densities that trigger…”
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The dependence of the evolution of Type Ia SN progenitors on the C-burning rate uncertainty and parameters of convective boundary mixing by Chen, Michael C., Herwig, Falk, Denissenkov, Pavel A., Paxton, Bill

“…Evolution of a Type Ia supernova (SN Ia) progenitor requires formation of a CO white dwarf (WD), which implies a dependence on the C-burning rate (CBR). It can…”
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Fast and Luminous Transients from the Explosions of Long-lived Massive White Dwarf Merger Remnants by Brooks, Jared, Schwab, Josiah, Bildsten, Lars, Quataert, Eliot, Paxton, Bill, Blinnikov, Sergei, Sorokina, Elena

“…We study the evolution and final outcome of long-lived ( years) remnants from the merger of an He white dwarf (WD) with a more massive C/O or O/Ne WD. Using…”
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Non-invasive prenatal chromosomal aneuploidy testing--clinical experience: 100,000 clinical samples by McCullough, Ron M, Almasri, Eyad A, Guan, Xiaojun, Geis, Jennifer A, Hicks, Susan C, Mazloom, Amin R, Deciu, Cosmin, Oeth, Paul, Bombard, Allan T, Paxton, Bill, Dharajiya, Nilesh, Saldivar, Juan-Sebastian

“…As the first laboratory to offer massively parallel sequencing-based noninvasive prenatal testing (NIPT) for fetal aneuploidies, Sequenom Laboratories has been…”
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THE RESPONSE OF GIANT STARS TO DYNAMICAL-TIMESCALE MASS LOSS by PASSY, Jean-Claude, HERWIG, Falk, PAXTON, Bill

“…We study the response of giant stars to mass loss. One-dimensional simulations of red and asymptotic giant branch stars with mass loss rates from 10 super(-3)…”
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EZ to Evolve ZAMS Stars: A Program Derived from Eggleton’s Stellar Evolution Code by Paxton, Bill

“…“Evolve ZAMS” (EZ) is a code derived from Peter Eggleton’s stellar evolution program. The core of EZ is a stripped down, rewritten version of a subset of…”
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Prolonged Central Nervous System Response in a Patient With HER2 Mutant NSCLC Treated With First-Line Poziotinib by Tchekmedyian, Nishan, Paxton, Bill, Lebel, Francois, Keossayan, Lena, Heymach, John V.

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ERRATUM: “HYDROGEN BURNING ON ACCRETING WHITE DWARFS: STABILITY, RECURRENT NOVAE, AND THE POST-NOVAE SUPERSOFT PHASE” (2013, ApJ, 777, 136) by Wolf, William M., Bildsten, Lars, Brooks, Jared, Paxton, Bill

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HYDROGEN BURNING ON ACCRETING WHITE DWARFS: STABILITY, RECURRENT NOVAE, AND THE POST-NOVA SUPERSOFT PHASE by Wolf, William M., Bildsten, Lars, Brooks, Jared, Paxton, Bill

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HYDROGEN BURNING ON ACCRETING WHITE DWARFS: STABILITY, RECURRENT NOVAE, AND THE POST-NOVA SUPERSOFT PHASE by Wolf, William M, Bildsten, Lars, Brooks, Jared, Paxton, Bill

“…We examine the properties of white dwarfs (WDs) accreting hydrogen-rich matter in and near the stable burning regime of accretion rates as modeled by…”
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Super-Eddington stellar winds driven by near-surface energy deposition by Quataert, Eliot, Fernández, Rodrigo, Kasen, Daniel, Klion, Hannah, Paxton, Bill

“…We develop analytic and numerical models of the properties of super-Eddington stellar winds, motivated by phases in stellar evolution when super-Eddington…”
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A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae by Goldberg, Jared A., Bildsten, Lars, Paxton, Bill

“…Massive stars undergo fundamental mode and first overtone radial pulsations with periods of 100-1000 days as red supergiants (RSGs). At large amplitudes, these…”
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AM CANUM VENATICORUM PROGENITORS WITH HELIUM STAR DONORS AND THE RESULTANT EXPLOSIONS by Brooks, Jared, Bildsten, Lars, Marchant, Pablo, Paxton, Bill

“…ABSTRACT We explore the outcome of mass transfer via Roche lobe overflow of pure helium burning stars in close binaries with WDs. The evolution is driven by…”
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MESA MODELS OF CLASSICAL NOVA OUTBURSTS: THE MULTICYCLE EVOLUTION AND EFFECTS OF CONVECTIVE BOUNDARY MIXING by DENISSENKOV, PAVEL A, Herwig, Falk, Bildsten, Lars, Paxton, Bill

“…Novae are cataclysmic variables driven by accretion of H-rich material onto a white dwarf (WD) star from its low-mass main-sequence binary companion. New…”
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Ellipsoidal Oscillations Induced by Substellar Companions: A Prospect for the Kepler Mission by Pfahl, Eric, Arras, Phil, Paxton, Bill

“…Hundreds of substellar companions to solar-type stars will be discovered with the Kepler satellite. Kepler's extreme photometric precision gives access to…”
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Modules for Experiments in Stellar Astrophysics (MESA) by Paxton, Bill, Bildsten, Lars, Dotter, Aaron L., Herwig, Falk, Lesaffre, Pierre, Timmes, Frank

“…Stellar physics and evolution calculations enable a broad range of research in astrophysics. Modules for Experiments in Stellar Astrophysics (MESA) is a suite…”
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