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19972021
most citedThe Supernova -- Gamma-Ray Burst Connection

1.8k citations · 5.7k across the 38 of their papers we have counts for

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Showing 2020Show all

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astro-ph.HE2020

Detection of Millihertz Quasi-Periodic Oscillations in the X-Ray Binary 1RXS J180408.9342058

Kaho Tse, Duncan K. Galloway, Yi Chou +2

Millihertz quasi-periodic oscillations (mHz QPOs) observed in neutron-star low-mass X-ray binaries (NS LMXBs) are generally explained as marginally stable thermonuclear burning on…

astro-ph.HE2020

The chemical signature of jet-driven hypernovae

J. J. Grimmett, Bernhard Müller, Alexander Heger +2

Hypernovae powered by magnetic jets launched from the surface of rapidly rotating millisecond magnetars are one of the leading models to explain broad-lined Type Ic supernovae (SNe…

astro-ph.HE202016 cited

The efficiency of nuclear burning during thermonuclear (Type I) bursts as a function of accretion rate

Y. Cavecchi, D. K. Galloway, A. J. Goodwin +2

We measured the thermonuclear burning efficiency as a function of accretion rate for the Type I X-ray bursts of five low-mass X-ray binary systems. We chose sources with measured n…

astro-ph.HE2020

Neutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network

K. Ackley, V. B. Adya, P. Agrawal +160

Gravitational waves from coalescing neutron stars encode information about nuclear matter at extreme densities, inaccessible by laboratory experiments. The late inspiral is influen…

astro-ph.GA202045 cited

A Minimum Dilution Scenario for Supernovae and Consequences for Extremely Metal-Poor Stars

Mattis Magg, Thomas Nordlander, Simon C. O. Glover +6

To date no metal-free stars have been identified by direct observations. The most common method of constraining their properties is searching the spectra of the most metal-poor sta…

astro-ph.HE2020146 cited

Three-dimensional Models of Core-collapse Supernovae From Low-mass Progenitors With Implications for Crab

G. Stockinger, H. -Th. Janka, D. Kresse +9

We present 3D full-sphere supernova simulations of non-rotating low-mass (~9 Msun) progenitors, covering the entire evolution from core collapse through bounce and shock revival, t…