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20082022
most citedCore-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions

1.1k citations · 3.2k across the 33 of their papers we have counts for

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19 papers · 1 filter

astro-ph.HE2021★ 37 cited

Comparing Compact Object Distributions from Mass- and Presupernova Core Structure-based Prescriptions

Rachel A. Patton, Tuguldur Sukhbold, J. J. Eldridge

Binary population synthesis (BPS) employs prescriptions to predict final fates, explosion or implosion, and remnant masses based on one or two stellar parameters at the evolutionar…

astro-ph.HE2020★ 45 cited

Model Light Curves for Type Ib and Ic Supernovae

Stan Woosley, Tuguldur Sukhbold, Daniel Kasen

Using the Monte Carlo code, SEDONA, multiband photometry and spectra are calculated for supernovae derived from stripped helium stars with presupernova masses from 2.2 to 10.0 $M_\…

astro-ph.HE2020★ 14 cited

ASASSN-18am/SN 2018gk : An overluminous Type IIb supernova from a massive progenitor

Subhash Bose, Subo Dong, C. S. Kochanek +29

ASASSN-18am/SN 2018gk is a newly discovered member of the rare group of luminous, hydrogen-rich supernovae (SNe) with a peak absolute magnitude of mag that is in…

astro-ph.HE2020★ 78 cited

The Birth Function for Black Holes and Neutron Stars in Close Binaries

S. Woosley, Tuguldur Sukhbold, H. -T. Janka

The mass function for black holes and neutron stars at birth is explored for mass-losing helium stars. These should resemble, more closely than similar studies of single hydrogen-r…

astro-ph.HE2019★ 189 cited

The Explosion of Helium Stars Evolved With Mass Loss

Thomas Ertl, Stan E. Woosley, Tuguldur Sukhbold +1

Light curves, explosion energies, and remnant masses are calculated for a grid of supernovae resulting from massive helium stars that have been evolved including mass loss. These p…

astro-ph.HE2019★ 17 cited

Probing the Innermost Ejecta Layers in SNR Kes 75: Implications for the Supernova Progenitor

Tea Temim, Patrick Slane, Tuguldur Sukhbold +3

Supernova remnants (SNRs) that contain pulsar wind nebulae (PWNe) are characterized by distinct evolutionary stages. In very young systems, the PWN drives a shock into the innermos…