activity
19952023
most citedA Non-Gray Theory of Extrasolar Giant Planets and Brown Dwarfs

1.4k citations · 36k across the 266 of their papers we have counts for

collaborators

268 papers

astro-ph.SR2023★ 1 cited

Black-Hole Formation Accompanied by the Supernova Explosion of a 40-M Progenitor Star

Adam Burrows, David Vartanyan, Tianshu Wang

We have simulated the collapse and evolution of the core of a solar-metallicity 40-M star and find that it explodes vigorously by the neutrino mechanism. This despite its…

astro-ph.HE2023★ 3 cited

Neutrino Signatures of One Hundred 2D Axisymmetric Core-Collapse Supernova Simulations

David Vartanyan, Adam Burrows

We present in this paper a public data release of an unprecedentedly-large set of core-collapse supernova (CCSN) neutrino emission models, comprising one hundred detailed 2D-axisym…

astro-ph.SR2023

Neutrino-Driven Winds in Three-Dimensional Core-Collapse Supernova Simulations

Tianshu Wang, Adam Burrows

In this paper, we analyze the neutrino-driven winds that emerge in twelve unprecedentedly long-duration 3D core-collapse supernova simulations done using the code Fornax. The twelv…

astro-ph.IM2023★ 17 cited

Measuring the properties of mode oscillations of a protoneutron star by third generation gravitational-wave detectors

Chaitanya Afle, Suman Kumar Kundu, Jenna Cammerino +4

Core-collapse supernovae are among the astrophysical sources of gravitational waves that could be detected by third-generation gravitational-wave detectors. Here, we analyze the gr…

astro-ph.EP2023★ 57 cited

Self-consistent Models of Y Dwarf Atmospheres with Water Clouds and Disequilibrium Chemistry

Brianna Lacy, Adam Burrows

Y dwarfs are the coolest spectral class of brown dwarf. They have effective temperatures less than 500 K, with the coolest detection as low as ~250 K. Their spectra are shaped pred…

astro-ph.HE2023★ 1 cited

The Gravitational-Wave Signature of Core-Collapse Supernovae

David Vartanyan, Adam Burrows, Tianshu Wang +2

We calculate the gravitational-wave (GW) signatures of detailed 3D core-collapse supernova simulations spanning a range of massive stars. Most of the simulations are carried out to…