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19972023
most citedImaging the Surface of Altair

331 citations · 7.7k across the 195 of their papers we have counts for

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astro-ph.SR2023★ 15 cited

VLTI/GRAVITY Observations and Characterization of the Brown Dwarf Companion HD 72946 B

W. O. Balmer, L. Pueyo, T. Stolker +96

Tension remains between the observed and modeled properties of substellar objects, but objects in binary orbits, with known dynamical masses can provide a way forward. HD 72946 B i…

astro-ph.SR2023

Refining the Stellar Parameters of Ceti: a Pole-on Solar Analog

Maria Korolik, Rachael M. Roettenbacher, Debra A. Fischer +16

To accurately characterize the planets a star may be hosting, stellar parameters must first be well-determined. Ceti is a nearby solar analog and often a target for exoplanet s…

astro-ph.SR2023★ 15 cited

The Great Dimming of the hypergiant star RW Cephei: CHARA Array images and spectral analysis

N. Anugu, F. Baron, D. R. Gies +15

The cool hypergiant star RW Cephei is currently in a deep photometric minimum that began several years ago. This event bears a strong similarity to the Great Dimming of the red sup…

astro-ph.SR2023★ 8 cited

Reconstructing the mid-infrared environment in the stellar merger remnant V838 Monocerotis

Muhammad Zain Mobeen, Tomasz Kamiński, Alexis Matter +15

V838 Mon is a stellar merger remnant that erupted in 2002 in a luminous red novae event. Although it is well studied in the optical, near infrared and submillimeter regimes, its st…

astro-ph.SR2023★ 7 cited

Imaging the warped dusty disk wind environment of SU Aurigae with MIRC-X

Aaron Labdon, Stefan Kraus, Claire L. Davies +12

SU Aurigae is a widely studied T Tauri star and here we present original state-of-the-art interferometric observations with better uv and baseline coverage than previous studies. W…

astro-ph.SR2023★ 10 cited

FU Orionis disk outburst: evidence for a gravitational instability scenario triggered in a magnetically dead zone

G. Bourdarot, J-P. Berger, G. Lesur +10

Context: FUors outbursts are a crucial stage of accretion in young stars. However a complete mechanism at the origin of the outburst still remains missing. Aims: We aim at constrai…