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20072023
most citedExoplanet Orbital Eccentricities Derived From LAMOST-Kepler Analysis

243 citations · 3.4k across the 74 of their papers we have counts for

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31 papers · 1 filter

astro-ph.SR2023

A Global 3-D Simulation of Magnetospheric Accretion: I. Magnetically Disrupted Disks and Surface Accretion

Zhaohuan Zhu, James M. Stone, Nuria Calvet

We present a 3-D ideal MHD simulation of magnetospheric accretion onto a non-rotating star. The accretion process unfolds with intricate 3-D structures driven by various mechanisms…

astro-ph.SR2023★ 8 cited

Resolving the Binary Components of the Outbursting Protostar HBC 494 with ALMA

Pedro Henrique Nogueira, Alice Zurlo, Sebastián Pérez +15

Episodic accretion is a low-mass pre-main sequence phenomenon characterized by sudden outbursts of enhanced accretion. These objects are classified into two: protostars with elevat…

astro-ph.SR2023★ 2 cited

Effective two-body scatterings around a massive object

Yihan Wang, Saavik Ford, Rosalba Perna +3

Two-body scatterings under the potential of a massive object are very common in astrophysics. If the massive body is far enough away that the two small bodies are in their own grav…

astro-ph.SR2020★ 40 cited

Large-scale CO spiral arms and complex kinematics associated with the T Tauri star RU Lup

Jane Huang, Sean M. Andrews, Karin I. Öberg +9

While protoplanetary disks often appear to be compact and well-organized in millimeter continuum emission, CO spectral line observations are increasingly revealing complex behavior…

astro-ph.SR2020★ 6 cited

A Study of Millimeter Variability in FUor Objects

John Wendeborn, Catherine C. Espaillat, Enrique Macias +6

FU Orionis objects (FUors) are rapidly-accreting, pre-main sequence objects that are known to exhibit large outbursts at optical and near-infrared wavelengths, with post-eruption,…

astro-ph.SR2020

A triple star system with a misaligned and warped circumstellar disk shaped by disk tearing

Stefan Kraus, Alexander Kreplin, Alison K. Young +29

Young stars are surrounded by a circumstellar disk of gas and dust, within which planet formation can occur. Gravitational forces in multiple star systems can disrupt the disk. The…