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20022026
most citedSPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations

757 citations · 12.6k across the 181 of their papers we have counts for

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Showing 2021Show all

16 papers · 1 filter

physics.space-ph2021★ 30 cited

Multi-spacecraft observations of the structure of the sheath of an interplanetary coronal mass ejection and related energetic ion enhancement

E. K. J. Kilpua, S. W. Good, N. Dresing +18

Sheaths ahead of coronal mass ejections (CMEs) are large heliospheric structures that form with CME expansion and propagation. Turbulent and compressed sheaths contribute to the ac…

astro-ph.EP2021★ 11 cited

The protoplanetary disc around HD 169142: circumstellar or circumbinary?

P. P. Poblete, N. Cuello, S. Pérez +12

Stellar binaries represent a substantial fraction of stellar systems, especially among young stellar objects. Accordingly, binaries play an important role in setting the architectu…

astro-ph.GA2021★ 34 cited

On the rise times in FU Orionis events

Elisabeth M. A. Borchert, Daniel J. Price, Christophe Pinte +1

We examine whether stellar flyby simulations can initiate FU Orionis outbursts using 3D hydrodynamics simulations coupled to live Monte Carlo radiative transfer. We find that a fly…

astro-ph.HE2021★ 19 cited

Gravitational waves from tidal disruption events: an open and comprehensive catalogue

Martina Toscani, Giuseppe Lodato, Daniel J. Price +1

We present an online, open and comprehensive template library of gravitational waveforms produced during the tidal disruptions of stars by massive black holes, spanning a broad spa…

astro-ph.EP2021★ 31 cited

Mapping the Planetary Wake in HD 163296 with Kinematics

Josh Calcino, Thomas Hilder, Daniel J. Price +4

We map the planetary wake associated with the embedded protoplanet creating the CO kink in the disk of HD~163296. We show that the wake can be traced by a series of correlated pert…

astro-ph.SR2021★ 79 cited

Common envelopes in massive stars: Towards the role of radiation pressure and recombination energy in ejecting red supergiant envelopes

Mike Y. M. Lau, Ryosuke Hirai, Miguel González-Bolívar +3

We perform 3D hydrodynamical simulations of a common-envelope event involving a 12 solar mass red supergiant donor. Massive stars are expected to be qualitatively different from lo…