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20032025
most citedOrigin of the heavy elements in binary neutron-star mergers from a gravitational wave event

1.2k citations · 30.2k across the 257 of their papers we have counts for

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Showing 2020Show all

19 papers · 1 filter

astro-ph.SR2020★ 18 cited

A "blue ring nebula" surrounding a thousands of years old stellar merger

Keri Hoadley, Christopher Martin, Brian D. Metzger +7

Stellar mergers are a brief-lived but common phase in the evolution of binary star systems. Among the many astrophysical implications of these events include the creation of atypic…

astro-ph.HE2020★ 177 cited

New Insights into Classical Novae

Laura Chomiuk, Brian D. Metzger, Ken J. Shen

We survey our understanding of classical novae: non-terminal, thermonuclear eruptions on the surfaces of white dwarfs in binary systems. The recent and unexpected discovery of GeV…

astro-ph.CO2020★ 71 cited

A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond

Hsin-Yu Chen, Philip S. Cowperthwaite, Brian D. Metzger +1

The most promising variation of the standard siren technique combines gravitational-wave (GW) data for binary neutron star (BNS) mergers with redshift measurements enabled by their…

astro-ph.SR2020★ 68 cited

The Stellar Merger Scenario for Black Holes in the Pair-instability Gap

M. Renzo, M. Cantiello, B. D. Metzger +1

The recent detection of GW190521 stimulated ideas on how to populate the predicted black hole pair-instability mass gap. One proposed scenario is the dynamical merger of two stars…

astro-ph.HE2020★ 12 cited

Fermi-LAT Observations of V549 Vel 2017: a Sub-Luminous Gamma-Ray Nova?

Kwan-Lok Li, Franz-Josef Hambsch, Ulisse Munari +4

We report on the Fermi-LAT detection (with ~5.7 sigma significance) as well as the multi-wavelength analysis of the 2017 nova eruption V549 Vel. Unlike the recent shock-powered nov…

astro-ph.HE2020★ 19 cited

Reconstructing Masses of Merging Neutron Stars from Stellar -Process Abundance Signatures

Erika M. Holmbeck, Anna Frebel, G. C. McLaughlin +5

Neutron star mergers (NSMs) are promising astrophysical sites for the rapid neutron-capture ("-") process, but can their integrated yields explain the majority of heavy-element…