8.6k citations · 29.5k across the 241 of their papers we have counts for
Showing 2018 · astro-ph.SRShow all
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astro-ph.SR2018★ 96 cited
The physical properties of AM CVn stars: new insights from Gaia DR2
G. Ramsay, M. J. Green, T. R. Marsh +9
AM CVn binaries are hydrogen deficient compact binaries with an orbital period in the 5-65 min range and are predicted to be strong sources of persistent gravitational wave radiati…
astro-ph.SR2018
Binaries as Sources of Gravitational Waves
Gijs Nelemans
With the discovery of both binary black hole mergers and a binary neutron star merger the field of Gravitational Wave Astrophysics has really begun. The current advanced LIGO and V…
astro-ph.SR2018★ 198 cited
LISA verification binaries with updated distances from Gaia Data Release 2
T. Kupfer, V. Korol, S. Shah +6
Ultracompact binaries with orbital periods less than a few hours will dominate the gravitational wave signal in the mHz regime. Until recently, 10 systems were expected have a pred…