papers

Publications (42)

astro-ph.SR2023

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.SR2025

The Dynamic Inner Disk of a Planet Forming Star

Benjamin R. Setterholm, John D. Monnier, Fabien Baron +13

Planets are a natural byproduct of the stellar formation process, resulting from local aggregations of material within the disks surrounding young stars. Whereas signatures of gas-…

astro-ph.EP2023

Three-dimensional orbit of AC Her determined: Binary-induced truncation cannot explain the large cavity in this post-AGB transition disk

Narsireddy Anugu, Jacques Kluska, Tyler Gardner +17

Some evolved binaries, namely post-asymptotic giant branch binaries, are surrounded by stable and massive circumbinary disks similar to protoplanetary disks found around young star…

astro-ph.SR2022

Scattering and sublimation: a multi-scale view of m-sized dust in the inclined disc of HD 145718

Claire L. Davies, Evan A. Rich, Tim J. Harries +15

We present multi-instrument observations of the disc around the Herbig~Ae star, HD~145718, employing geometric and Monte Carlo radiative transfer models to explore the disc orienta…

astro-ph.EP2021

EXPRES. III. Revealing the Stellar Activity Radial Velocity Signature of Eridani with Photometry and Interferometry

Rachael M. Roettenbacher, Samuel H. C. Cabot, Debra A. Fischer +20

The distortions of absorption line profiles caused by photospheric brightness variations on the surfaces of cool, main-sequence stars can mimic or overwhelm radial velocity (RV) sh…

astro-ph.IM2020

MIRC-X: a highly-sensitive six telescope interferometric imager at the CHARA Array

Narsireddy Anugu, Jean-Baptiste Le Bouquin, John D. Monnier +11

MIRC-X (Michigan InfraRed Combiner-eXeter) is a new highly-sensitive six-telescope interferometric imager installed at the CHARA Array that provides an angular resolution equivalen…

astro-ph.EP2025

Surprise non-detection of Upsilon Andromedae b with MIRC-X and MYSTIC at the CHARA Array

Tyler Gardner, John D. Monnier, Stefan Kraus +11

Ground-based long baseline interferometry is a powerful tool for characterizing exoplanets which are too close to their host star to be imaged with single-dish telescopes. The CHAR…

astro-ph.SR2024

Visual Orbits of Wolf-Rayet Stars I: The Orbit of the dust-producing Wolf-Rayet binary WR\,137 measured with the CHARA Array

Noel D. Richardson, Gail H. Schaefer, Jan J. Eldridge +19

Classical Wolf-Rayet stars are the descendants of massive OB stars that have lost their hydrogen envelopes and are burning helium in their cores prior to exploding as type Ib/c sup…

astro-ph.SR2023

Multiplicity of northern bright O-type stars with optical long baseline interferometry

Cyprien Lanthermann, Jean-Baptiste Le Bouquin, Hugues Sana +16

The study of the multiplicity of massive stars gives hints on their formation processes and their evolutionary paths, which are still not fully understood. Large separation binarie…

astro-ph.SR2025

Precise Age For The Binary HD 21278 In The Young Alpha Persei Cluster

Christopher A. Danner, Eric L. Sandquist, Gail H. Schaefer +14

We present a study of the double-lined spectroscopic binary HD 21278 that contains one of the brightest main sequence stars in the young Persei open cluster. We analyzed new s…

astro-ph.SR2023

Orbits and Dynamical Masses for the Active Hyades Multiple System HD 284163

Guillermo Torres, Gail H. Schaefer, Robert P. Stefanik +16

We report near-infrared long-baseline interferometric observations of the Hyades multiple system HD 284163, made with the CHARA array, as well as almost 43 yr of high-resolution sp…

astro-ph.IM2022

High spectral-resolution interferometry down to 1 micron with Asgard/BIFROST at VLTI: Science drivers and project overview

Stefan Kraus, Daniel Mortimer, Sorabh Chhabra +10

We present science cases and instrument design considerations for the BIFROST instrument that will open the short-wavelength (Y/J/H-band), high spectral dispersion (up to R=25,000)…

astro-ph.EP2020

Spin-orbit alignment of the Pictoris planetary system

Stefan Kraus, Jean-Baptiste LeBouquin, Alexander Kreplin +6

A crucial diagnostic that can tell us about processes involved in the formation and dynamical evolutionof planetary systems is the angle between the rotation axis of a star and a p…

astro-ph.SR2022

The Orbits and Dynamical Masses of the Castor System

Guillermo Torres, Gail H. Schaefer, John D. Monnier +12

Castor is a system of six stars in which the two brighter objects, Castor A and B, revolve around each other every 450 yr and are both short-period spectroscopic binaries. Th…

astro-ph.SR2025

The Small Separation A-Star Companion Population: Tentative Signatures of Enhanced Multiplicity with Primary Mass

Matthew De Furio, Tyler Gardner, John D. Monnier +6

We present updated results from our near-infrared long-baseline interferometry (LBI) survey to constrain the multiplicity properties of intermediate-mass A-type stars within 80 pc.…

astro-ph.SR2024

Time-Evolution Images of the Hypergiant RW Cephei During the Re-brightening Phase Following the Great Dimming

Narsireddy Anugu, Douglas R. Gies, Rachael M. Roettenbacher +17

Stars with initial masses larger than 8 solar masses undergo substantial mass loss through mechanisms that remain elusive. Unraveling the origins of this mass loss is important for…

astro-ph.SR2022

The Interferometric Binary Epsilon Cancri in Praesepe: Precise Masses and Age

Leslie M. Morales, Eric L. Sandquist, Gail H. Schaefer +16

We observe the brightest member of the Praesepe cluster, Epsilon Cancri, to precisely measure the characteristics of the stars in this binary system, en route to a new measurement…

astro-ph.SR2024

Visual Orbits of Wolf-Rayet Stars II: The Orbit of the Nitrogen-Rich WR Binary WR 138 measured with the CHARA Array

Amanda Holdsworth, Noel Richardson, Gail H. Schaefer +19

Classical Wolf-Rayet stars are descendants of massive OB-type stars that have lost their hydrogen-rich envelopes, and are in the final stages of stellar evolution, possibly explodi…

astro-ph.SR2018

Precision Orbit of Delphini and Prospects for Astrometric Detection of Exoplanets

Tyler Gardner, John D. Monnier, Francis C. Fekel +17

Combining visual and spectroscopic orbits of binary stars leads to a determination of the full 3D orbit, individual masses, and distance to the system. We present a full analysis o…

astro-ph.IM2024

Pushing high angular resolution and high contrast observations on the VLTI from Y to L band with the Asgard instrumental suite: integration status and plans

Marc-Antoine Martinod, Denis Defrère, Michael J. Ireland +35

ESO's Very Large Telescope Interferometer has a history of record-breaking discoveries in astrophysics and significant advances in instrumentation. The next leap forward is its new…

astro-ph.SR2022

Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692

Kathryn V. Lester, Gail H. Schaefer, Francis C. Fekel +18

We present the visual orbits of four spectroscopic binary stars, HD 61859, HD 89822, HD 109510, and HD 191692, using long baseline interferometry with the CHARA Array. We also obta…

astro-ph.SR2022

Characterising the orbit and circumstellar environment of the high-mass binary MWC 166 A

Sebastian A. Zarrilli, Stefan Kraus, Alexander Kreplin +13

Context: Stellar evolution models are highly dependent on accurate mass estimates, especially for high-mass stars in the early stages of evolution. The most direct method for obtai…

astro-ph.SR2021

Gem: a hierarchical triple system with an outer Be star

Robert Klement, Petr Hadrava, Thomas Rivinius +17

Time series of spectroscopic, speckle-interferometric, and optical long-baseline-interferometric observations confirm that Gem is a hierarchical triple system. It consists of…

astro-ph.SR2022

ARMADA II: Further Detections of Inner Companions to Intermediate Mass Binaries with Micro-Arcsecond Astrometry at CHARA and VLTI

Tyler Gardner, John D. Monnier, Francis C. Fekel +18

We started a survey with CHARA/MIRC-X and VLTI/GRAVITY to search for low mass companions orbiting individual components of intermediate mass binary systems. With the incredible pre…

astro-ph.SR2021

The First Dynamical Mass Determination of a Nitrogen-rich Wolf-Rayet Star using a Combined Visual and Spectroscopic Orbit

Noel D. Richardson, Laura Lee, Gail Schaefer +11

We present the first visual orbit for the nitrogen-rich Wolf-Rayet binary, WR 133 (WN5o + O9I) based on observations made with the CHARA Array and the MIRC-X combiner. This orbit r…

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…

astro-ph.EP2023

ACCESS, LRG-BEASTS, & MOPSS: Featureless Optical Transmission Spectra of WASP-25b and WASP-124b

Chima D. McGruder, Mercedes López-Morales, James Kirk +14

We present new optical transmission spectra for two hot Jupiters: WASP-25b (M = 0.56~M; R = 1.23 R; P =~3.76 days) and WASP-124b (M = 0.58~M; R = 1.34 R; P = 3.37 d…

astro-ph.SR2022

The Small Separation A-Star Companion Population: First Results with CHARA/MIRC-X

Matthew De Furio, Tyler Gardner, John Monnier +9

We present preliminary results from our long-baseline interferometry (LBI) survey to constrain the multiplicity properties of intermediate-mass A-type stars within 80pc. Previous m…

astro-ph.SR2020

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.SR2023

Imaging the inner astronomical unit of Herbig Be star HD 190073

Nour Ibrahim, John D. Monnier, Stefan Kraus +13

Inner regions of protoplanetary disks host many complex physical processes such as star-disk interactions, magnetic fields, planet formation, and the migration of new planets. To d…

astro-ph.IM2020

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.HE2025

Multiple outflows and delayed ejections revealed by early imaging of novae

Elias Aydi, John D. Monnier, Antoine Mérand +39

Novae are thermonuclear eruptions on accreting white dwarfs in interacting binaries. Although most of the accreted envelope is expelled, the mechanism -- impulsive ejection, multip…

astro-ph.SR2023

The CHARA Array interferometric program on the multiplicity of classical Be stars: new detections and orbits of stripped subdwarf companions

Robert Klement, Thomas Rivinius, Douglas R. Gies +8

Rapid rotation and nonradial pulsations enable Be stars to build decretion disks, where the characteristic line emission forms. A major but unconstrained fraction of Be stars owe t…

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…

astro-ph.SR2021

Establishing Oph as a Prototype Rotator: Precision Orbit with new Keck, CHARA, and RV Observations

Tyler Gardner, John D. Monnier, Francis C. Fekel +11

Alpha Ophiuchi (Rasalhague) is a nearby rapidly rotating A5IV star which has been imaged by infrared interferometry. Oph is also part of a known binary system, with a companio…

astro-ph.SR2026

Pre-nova Observations of T CrB: A view from the CHARA Array

Ryan Norris, Narsireddy Anugu, Thomas Gaudin +38

T CrB is a symbiotic recurrent nova consisting of a red giant and white dwarf with recent eruptions in 1866 and 1946 and an anticipated eruption in the mid 2020s. We report CHARA A…

astro-ph.SR2023

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

Precise Age for the Binary Star System 12 Com in the Coma Berenices Cluster

Rex Lam, Eric L. Sandquist, Gail H. Schaefer +11

We present measurements of the interferometrically-resolved binary star system 12 Com and the single giant star 31 Com in the cluster Coma Berenices. 12 Com is a double-lined spect…

astro-ph.SR2026

Interferometric Images of the Starspot Evolution of Andromedae

Rachael M. Roettenbacher, John D. Monnier, Heidi Korhonen +21

The evolution of starspots of the giant primaries of RS CVn systems is typically detected indirectly with photometric and spectroscopic monitoring. These observations suggest slowl…

astro-ph.IM2025

The CHARA Array Polarization Model and Prospects for Spectropolarimetry

Linling Shuai, John D. Monnier, Benjamin R. Setterholm +5

Polarimetric data provide key insights into infrared emission mechanisms in the inner disks of YSOs and the details of dust formation around AGB stars. While polarization measureme…

astro-ph.SR2024

CHARA Near-Infrared Imaging of the Yellow Hypergiant Star Cassiopeiae: Convection Cells and Circumstellar Envelope

Narsireddy Anugu, Fabien Baron, John D. Monnier +18

Massive evolved stars such as red supergiants and hypergiants are potential progenitors of Type II supernovae, and they are known for ejecting substantial amounts of matter, up to…

astro-ph.SR2021

The orbit and stellar masses of the archetype colliding-wind binary WR 140

Joshua D. Thomas, Noel D. Richardson, J. J. Eldridge +33

We present updated orbital elements for the Wolf-Rayet (WR) binary WR\,140 (HD\,193793; WC7pd + O5.5fc). The new orbital elements were derived using previously published measuremen…