activity
19972023
most citedImaging the Surface of Altair

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

collaborators
Showing 2020Show all

17 papers · 1 filter

astro-ph.IM2020★ 9 cited

CHARA Array adaptive optics: complex operational software and performance

Narsireddy Anugu, Theo ten Brummelaar, Nils H. Turner +18

The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural seeing, it has delivered landmark sub-milliarcsecond results in the areas of stel…

astro-ph.IM2020★ 3 cited

CHARA/MIRC-X -- a high-sensitive six telescope interferometric imager concept, commissioning, and early science

Narsireddy Anugu, Jean-Baptiste Le Bouquin, John D. Monnier +14

MIRC-X is a six telescope beam combiner at the CHARA array that works in J and H wavelength bands and provides an angular resolution equivalent to a =331m diameter telescope. Th…

astro-ph.SR2020★ 3 cited

VLTI images of circumbinary disks around evolved stars

Jacques Kluska, Rik Claes, Akke Corporaal +13

The new generation of VLTI instruments (GRAVITY, MATISSE) aims to produce routinely interferometric images to uncover the morphological complexity of different objects at high angu…

astro-ph.IM2020

A New Frontier for J-band Interferometry: Dual-band NIRInterferometry with MIRC-X

Aaron Labdon, John D. Monnier, Stefan Kraus +11

In this contribution we report on our work to increase the spectral range of the Michigan Infrared Combiner-eXeter (MIRC-X) instrument at the CHARA array to allow for dual H and J…

astro-ph.SR2020★ 16 cited

ARMADA I: Triple Companions Detected in B-Type Binaries alpha Del and nu Gem

Tyler Gardner, John D. Monnier, Francis C. Fekel +19

Ground-based optical long-baseline interferometry has the power to measure the orbits of close binary systems at ~10 micro-arcsecond precision. This precision makes it possible to…

astro-ph.SR2020★ 23 cited

Viscous Heating and Boundary Layer Accretion in the Disk of Outbursting Star FU Orionis

Aaron Labdon, Stefan Kraus, Claire L Davies +11

Context. FU Orionis is the archetypal FUor star, a subclass of young stellar object (YSO) that undergo rapid brightening events, often gaining 4-6 magnitudes on timescales of days.…