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20012025
most citedOrigin of the heavy elements in binary neutron-star mergers from a gravitational wave event

1.2k citations · 21.4k across the 157 of their papers we have counts for

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15 papers · 1 filter

astro-ph.SR2022

StaNdaRT: A repository of standardized test models and outputs for supernova radiative transfer

Stéphane Blondin, Sergei Blinnikov, Fionntan P. Callan +26

We present the first results of a comprehensive supernova (SN) radiative-transfer (RT) code-comparison initiative (StaNdaRT), where the emission from the same set of standardized t…

astro-ph.SR2022★ 20 cited

3D Hydrodynamics of Pre-supernova Outbursts in Convective Red Supergiant Envelopes

Benny T. -H. Tsang, Daniel Kasen, Lars Bildsten

Eruptive mass loss likely produces the energetic outbursts observed from some massive stars before they undergo core-collapse supernovae (CCSNe). The resulting dense circumstellar…

astro-ph.SR2021★ 65 cited

Multi-Dimensional Radiative Transfer Calculations of Double Detonations of Sub-Chandrasekhar-Mass White Dwarfs

Ken J. Shen, Samuel J. Boos, Dean M. Townsley +1

Study of the double detonation Type Ia supernova scenario, in which a helium shell detonation triggers a carbon core detonation in a sub-Chandrasekhar-mass white dwarf, has experie…

astro-ph.SR2019★ 100 cited

Double Detonations with Thin, Modestly Enriched Helium Layers Can Make Normal Type Ia Supernovae

Dean M. Townsley, Broxton J. Miles, Ken J. Shen +1

It has been proposed that Type Ia supernovae (SNe Ia) that are normal in their spectra and brightness can be explained by a double detonation that ignites first in a helium shell o…

astro-ph.SR2018★ 85 cited

Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the 2 Observations

W. Li, X. Wang, J. Vinkó +160

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the field. The data revealed an excess emission…

astro-ph.SR2017★ 67 cited

Multidimensional Models of Type Ia Supernova Nebular Spectra: Strong Emission Lines from Stripped Companion Gas Rule Out Classic Single Degenerate Systems

Janos Botyanszki, Daniel Kasen, Tomasz Plewa

The classic single-degenerate model for the progenitors of Type Ia Supernova (SN Ia) predicts that the supernova ejecta should be enriched with solar-like abundance material stripp…

astro-ph.SR2016★ 8 cited

Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times

Brian Friesen, E. Baron, Jerod T. Parrent +16

We present optical spectra of the nearby Type Ia supernova SN 2011fe at 100, 205, 311, 349, and 578 days post-maximum light, as well as an ultraviolet spectrum obtained with Hubble…

astro-ph.SR2016★ 113 cited

The Evolution and Fate of Super-Chandrasekhar Mass White Dwarf Merger Remnants

Josiah Schwab, Eliot Quataert, Daniel Kasen

We present stellar evolution calculations of the remnant of the merger of two carbon-oxygen white dwarfs (CO WDs). We focus on cases that have a total mass in excess of the Chandra…

astro-ph.SR2016★ 91 cited

Shock Breakout and Early Light Curves of Type II-P Supernovae Observed with Kepler

P. M. Garnavich, B. E. Tucker, A. Rest +4

We discovered two transient events in the Kepler field with light curves that strongly suggest they are type II-P supernovae. Using the fast cadence of the Kepler observations we p…

astro-ph.SR2015★ 119 cited

Super-Eddington Stellar Winds Driven by Near-Surface Energy Deposition

Eliot Quataert, Rodrigo Fernandez, Daniel Kasen +2

We develop analytic and numerical models of the properties of super-Eddington stellar winds, motivated by phases in stellar evolution when super-Eddington energy deposition (via, e…

astro-ph.SR2011★ 118 cited

XRF 100316D / SN 2010bh and the Nature of Gamma Ray Burst Supernovae

Z. Cano, D. Bersier, C. Guidorzi +21

We present ground-based and HST optical and infrared observations of XRF 100316D / SN 2010bh. It is seen that the optical light curves of SN 2010bh evolve at a faster rate than the…

astro-ph.SR2010★ 118 cited

Direct Confirmation of the Asymmetry of the Cas A Supernova with Light Echoes

A. Rest, R. J. Foley, B. Sinnott +21

We report the first detection of asymmetry in a supernova (SN) photosphere based on SN light echo (LE) spectra of Cas A from the different perspectives of dust concentrations on it…

astro-ph.SR2010

Modeling the Diversity of Type Ia Supernova Explosions

F. K. Roepke, W. Hillebrandt, D. Kasen +1

Type Ia supernovae (SNe Ia) are a prime tool in observational cosmology. A relation between their peak luminosities and the shapes of their light curves allows to infer their intri…

astro-ph.SR2009★ 2 cited

Monte Carlo Radiative Transfer Simulations: Applications to Astrophysical Outflows and Explosions

S. A. Sim, M. Kromer, F. K. Roepke +4

The theory of radiative transfer provides the link between the physical conditions in an astrophysical object and the observable radiation which it emits. Thus accurately modelling…

astro-ph.SR2009★ 11 cited

Type Ia supernova science 2010-2020

D. A. Howell, A. Conley, M. Della Valle +47

In the next decade Type Ia supernovae (SNe Ia) will be used to test theories predicting changes in the Dark Energy equation of state with time. Ultimately this requires a dedicated…