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TURBOVELOCITY STARS: KICKS RESULTING FROM THE TIDAL DISRUPTION OF SOLITARY STARS

Astrophysical journal. Letters, 2013-06, Vol.771 (2), p.L28

2013

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SIMULATIONS OF GAMMA-RAY BURST JETS IN A STRATIFIED EXTERNAL MEDIUM: DYNAMICS, AFTERGLOW LIGHT CURVES, JET BREAKS, AND RADIO CALORIMETRY

The Astrophysical journal, 2012-05, Vol.751 (1), p.57

2012

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ON THE ACCRETION-FED GROWTH OF NEUTRON STARS DURING COMMON ENVELOPE

Astrophysical journal. Letters, 2014-12, Vol.798 (1), p.L19

2014

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GAMMA-RAY BURST DYNAMICS AND AFTERGLOW RADIATION FROM ADAPTIVE MESH REFINEMENT, SPECIAL RELATIVISTIC HYDRODYNAMIC SIMULATIONS

The Astrophysical journal, 2012-02, Vol.746 (2), p.122

2012

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The White Dwarf Initial–Final Mass Relation for Progenitor Stars from 0.85 to 7.5 M

The Astrophysical journal, 2018-10, Vol.866 (1), p.21

2018

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PS1-10jh: THE DISRUPTION OF A MAIN-SEQUENCE STAR OF NEAR-SOLAR COMPOSITION

The Astrophysical journal, 2014-02, Vol.783 (1), p.23

2014

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Transients stemming from collapsing massive stars: The missing pieces to advance joint observations of photons and high-energy neutrinos

Physical review. D, 2023-10, Vol.108 (8), Article 083035

2023

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ERRATUM: “HYDRODYNAMICAL SIMULATIONS TO DETERMINE THE FEEDING RATE OF BLACK HOLES BY THE TIDAL DISRUPTION OF STARS: THE IMPORTANCE OF THE IMPACT PARAMETER AND STELLAR STRUCTURE” (2013, ApJ, 767, 25)

The Astrophysical journal, 2015-01, Vol.798 (1), p.64

2015

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A Possible Cepheid-like Luminosity Estimator for the Long Gamma-Ray Bursts

The Astrophysical journal, 2001-05, Vol.552 (1), p.57-71

2001

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TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL–FINAL MASS RELATION FOR PROGENITORS OF 4–6.5 M

The Astrophysical journal, 2016-02, Vol.818 (1), p.84

2016

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THE ROLE OF STELLAR FEEDBACK IN THE DYNAMICS OF HII REGIONS

The Astrophysical journal, 2014-01, Vol.795 (2), p.1-18

2014

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The Stars in M15 Were Born with the r-process The data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation

Astrophysical journal. Letters, 2020-03, Vol.891 (1)

2020

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INITIAL–FINAL MASS RELATION FOR 3 TO 4 M ⊙ PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099

The Astrophysical journal, 2015-07, Vol.807 (1), p.90

2015

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The White Dwarf Initial-Final Mass Relation for Progenitor Stars from 0.85 to 7.5 M Based on observations with the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, was made possible by the generous financial support of the W.M. Keck Foundation

The Astrophysical journal, 2018-10, Vol.866 (1)

2018

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Erratum: "Optical Thermonuclear Transients From Tidal Compression of White Dwarfs as Tracers of the Low End of the Massive Black Hole Mass Function" (2016, ApJ, 819, 3)

The Astrophysical journal, 2017-07, Vol.843 (2), p.154

2017

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A Survey for N V Absorption at z zGRB in GRB Afterglow Spectra: Clues to Gas Near the Progenitor Star

The Astrophysical journal, 2008-09, Vol.685 (1), p.344-353

2008

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TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL-FINAL MASS RELATION FOR PROGENITORS OF 4-6.5 M sub([middot in circle])

The Astrophysical journal, 2016-02, Vol.818 (1)

2016

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TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL-FINAL MASS RELATION FOR PROGENITORS OF 4-6.5 M Based on observations with the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, was made possible by the generous financial support of the W.M. Keck Foundation

The Astrophysical journal, 2016-02, Vol.818 (1)

2016

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THE TIDAL DISRUPTION OF GIANT STARS AND THEIR CONTRIBUTION TO THE FLARING SUPERMASSIVE BLACK HOLE POPULATION

The Astrophysical journal, 2012, Vol.755 (2)

2012

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THE FATE OF THE COMPACT REMNANT IN NEUTRON STAR MERGERS

The Astrophysical journal, 2015-10, Vol.812 (1)

2015

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INITIAL-FINAL MASS RELATION FOR 3 TO 4 M PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099 Based on observations with the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA and was made possible by the generous financial support of the W. M. Keck Foundation

The Astrophysical journal, 2015-07, Vol.807 (1)

2015

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INITIAL-FINAL MASS RELATION FOR 3 TO 4 M sub([middot in circle]) PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099

The Astrophysical journal, 2015-07, Vol.807 (1), p.1-12

2015

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Maybe not so old after all

Nature (London), 2009-08, Vol.460 (7259), p.1091-1092

2009

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AN ULTRAMASSIVE 1.28 M ⊙ WHITE DWARF IN NGC 2099

Astrophysical journal. Letters, 2016-03, Vol.820 (1), p.L18

2016

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AN ULTRAMASSIVE 1.28 M sub([middot in circle]) WHITE DWARF IN NGC 2099

Astrophysical journal. Letters, 2016-03, Vol.820 (1), p.L18-L18

2016

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TURBOVELOCITY STARS: KICKS RESULTING FROM THE TIDAL DISRUPTION OF SOLITARY STARS

SIMULATIONS OF GAMMA-RAY BURST JETS IN A STRATIFIED EXTERNAL MEDIUM: DYNAMICS, AFTERGLOW LIGHT CURVES, JET BREAKS, AND RADIO CALORIMETRY

ON THE ACCRETION-FED GROWTH OF NEUTRON STARS DURING COMMON ENVELOPE

GAMMA-RAY BURST DYNAMICS AND AFTERGLOW RADIATION FROM ADAPTIVE MESH REFINEMENT, SPECIAL RELATIVISTIC HYDRODYNAMIC SIMULATIONS

The White Dwarf Initial–Final Mass Relation for Progenitor Stars from 0.85 to 7.5 M

PS1-10jh: THE DISRUPTION OF A MAIN-SEQUENCE STAR OF NEAR-SOLAR COMPOSITION

Transients stemming from collapsing massive stars: The missing pieces to advance joint observations of photons and high-energy neutrinos

ERRATUM: “HYDRODYNAMICAL SIMULATIONS TO DETERMINE THE FEEDING RATE OF BLACK HOLES BY THE TIDAL DISRUPTION OF STARS: THE IMPORTANCE OF THE IMPACT PARAMETER AND STELLAR STRUCTURE” (2013, ApJ, 767, 25)

A Possible Cepheid-like Luminosity Estimator for the Long Gamma-Ray Bursts

TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL–FINAL MASS RELATION FOR PROGENITORS OF 4–6.5 M

THE ROLE OF STELLAR FEEDBACK IN THE DYNAMICS OF HII REGIONS

INITIAL–FINAL MASS RELATION FOR 3 TO 4 M ⊙ PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099

Erratum: "Optical Thermonuclear Transients From Tidal Compression of White Dwarfs as Tracers of the Low End of the Massive Black Hole Mass Function" (2016, ApJ, 819, 3)

A Survey for N V Absorption at z zGRB in GRB Afterglow Spectra: Clues to Gas Near the Progenitor Star

TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL-FINAL MASS RELATION FOR PROGENITORS OF 4-6.5 M sub([middot in circle])

THE TIDAL DISRUPTION OF GIANT STARS AND THEIR CONTRIBUTION TO THE FLARING SUPERMASSIVE BLACK HOLE POPULATION

THE FATE OF THE COMPACT REMNANT IN NEUTRON STAR MERGERS

INITIAL-FINAL MASS RELATION FOR 3 TO 4 M sub([middot in circle]) PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099

Maybe not so old after all

AN ULTRAMASSIVE 1.28 M ⊙ WHITE DWARF IN NGC 2099

AN ULTRAMASSIVE 1.28 M sub([middot in circle]) WHITE DWARF IN NGC 2099

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