activity
20092026
most citedRotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones

888 citations · 11.1k across the 129 of their papers we have counts for

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Showing 2021Show all

10 papers · 1 filter

astro-ph.HE2021

Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties

Floor S. Broekgaarden, Edo Berger, Simon Stevenson +9

Making the most of the rapidly increasing population of gravitational-wave detections of black hole (BH) and neutron star (NS) mergers requires comparing observations with populati…

astro-ph.SR2021★ 88 cited

Detailed models of interacting short-period massive binary stars

K. Sen, N. Langer, P. Marchant +10

About a quarter of massive binary stars undergo mass transfer while both stars burn hydrogen at their cores, first on the thermal and then on the nuclear timescale. The nuclear tim…

astro-ph.HE2021★ 54 cited

Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA

Tom Wagg, Floor S. Broekgaarden, Selma E. de Mink +3

Future searches for gravitational waves from space will be sensitive to double compact objects (DCOs) in our Milky Way. We present new simulations of the populations of double blac…

astro-ph.HE2021★ 37 cited

LEGWORK: A python package for computing the evolution and detectability of stellar-origin gravitational-wave sources with space-based detectors

Tom Wagg, Katelyn Breivik, Selma E. de Mink

We present LEGWORK (LISA Evolution and Gravitational Wave Orbit Kit), an open-source Python package for making predictions about stellar-origin gravitational wave sources and their…

astro-ph.SR2021★ 34 cited

The cosmic carbon footprint of massive stars stripped in binary systems

R. Farmer, E. Laplace, S. E. de Mink +1

The cosmic origin of carbon, a fundamental building block of life, is still uncertain. Yield predictions for massive stars are almost exclusively based on single star models, even…

astro-ph.HE2021★ 152 cited

The redshift evolution of the binary black hole merger rate: a weighty matter

L. A. C. van Son, S. E. de Mink, T. Callister +7

Gravitational wave detectors are starting to reveal the redshift evolution of the binary black hole (BBH) merger rate, . We make predictions for $R_{\mathrm{BB…

astro-ph.IM2021★ 3 cited

Rapid stellar and binary population synthesis with COMPAS

Team COMPAS, :, Jeff Riley +23

Compact Object Mergers: Population Astrophysics and Statistics (COMPAS; https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of…

astro-ph.SR2021★ 42 cited

The B-type Binaries Characterisation Programme I. Orbital solutions for the 30 Doradus population

J. I. Villaseñor, W. D. Taylor, C. J. Evans +6

We present results from the B-type Binaries Characterisation (BBC) programme, a multi-epoch spectroscopic study of 88 early B-type binary candidates in the 30 Doradus region of the…

astro-ph.HE2021★ 156 cited

Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers

Floor S. Broekgaarden, Edo Berger, Coenraad J. Neijssel +7

Mergers of black hole-neutron star (BHNS) binaries have now been observed by GW detectors with the recent announcement of GW200105 and GW200115. Such observations not only provide…

astro-ph.SR2021★ 160 cited

Different to the core: the pre-supernova structures of massive single and binary-stripped stars

E. Laplace, S. Justham, M. Renzo +4

The majority of massive stars live in binary or multiple systems and will interact during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae…