papers

Publications (30)

astro-ph.SR2018

The convective photosphere of the red supergiant CE Tau. I. VLTI/PIONIER H-band interferometric imaging

M. Montargès, R. Norris, A. Chiavassa +3

Context. Red supergiant stars are one of the latest stages in the evolution of massive stars. Their photospheric convection may play an important role in the launching mechanism of…

astro-ph.SR2020

VLTI-PIONIER imaging of the red supergiant V602 Carinae

J. B. Climent, M. Wittkowski, A. Chiavassa +7

Context. Red supergiant stars possess surface features and extended molecular atmospheres. Photospheric convection may be a crucial factor of the levitation of the outer atmospheri…

astro-ph.SR2023

A long-term study of the magnetic field and activity in the M giant RZ Ari

R. Konstantinova-Antova, S. Georgiev, A. Lèbre +12

We present a detailed long-term study of the single M6 III giant RZ~Ari to obtain direct and simultaneous measurements of the magnetic field, activity indicators, and radial veloci…

astro-ph.SR2025

An accreting dwarf star orbiting the S-type giant star pi1 Gru

M. Montargès, J. Malfait, M. Esseldeurs +20

Aims. We aim to characterize the properties of the inner companion of the S-type AGB star pi1 Gru and to identify plausible future evolutionary scenarios for this triple system. Me…

astro-ph.SR2012

Resolving Vega and the inclination controversy with CHARA/MIRC

J. D. Monnier, Xiao Che, Ming Zhao +15

Optical and infrared interferometers definitively established that the photometric standard Vega (alpha Lyrae) is a rapidly rotating star viewed nearly pole-on. Recent independent…

astro-ph.SR2016

Orbits, Distance, and Stellar Masses of the Massive Triple Star Sigma Orionis

G. H. Schaefer, C. A. Hummel, D. R. Gies +11

We present interferometric observations of the sigma Orionis triple system using the CHARA Array, NPOI, and VLTI. Using these measurements, we spatially resolve the orbit of the cl…

astro-ph2008

Discovery of a Circumbinary Disk around Herbig Ae/Be system v892 Tau

J. D. Monnier, A. Tannirkulam, P. G. Tuthill +4

We report the discovery of a circumbinary disk around the Herbig Ae/Be system v892 Tau. Our detailed mid-infrared images were made using segment-tilting interferometry on the Keck-…

astro-ph.SR2015

The Expanding Fireball of Nova Delphini 2013

G. H. Schaefer, T. ten Brummelaar, D. R. Gies +34

A classical nova occurs when material accreting onto the surface of a white dwarf in a close binary system ignites in a thermonuclear runaway. Complex structures observed in the ej…

astro-ph.SR2011

First visual orbit for the prototypical colliding-wind binary WR 140

J. D. Monnier, Ming Zhao, E. Pedretti +14

Wolf-Rayet stars represent one of the final stages of massive stellar evolution. Relatively little is known about this short-lived phase and we currently lack reliable mass, distan…

astro-ph.SR2012

Imaging the Algol Triple System in H Band with the CHARA Interferometer

F. Baron, J. D. Monnier, E. Pedretti +12

Algol (Beta Per) is an extensively studied hierarchical triple system whose inner pair is a prototype semi-detached binary with mass transfer occurring from the sub-giant secondary…

astro-ph2008

First Resolved Images of the Eclipsing and Interacting Binary Beta Lyrae

M. Zhao, D. Gies, J. D. Monnier +12

We present the first resolved images of the eclipsing binary Beta Lyrae, obtained with the CHARA Array interferometer and the MIRC combiner in the H band. The images clearly show t…

astro-ph.SR2017

Asymmetries on red giant branch surfaces from CHARA/MIRC optical interferometry

A. Chiavassa, R. Norris, M. Montargès +14

Context. Red giant branch (RGB) stars are very bright objects in galaxies and are often used as standard candles. Interferometry is the ideal tool to characterize the dynamics and…

astro-ph.SR2024

An impressionist view of V Hydrae. When MATISSE paints Asymmetric Giant Blobs

L. Planquart, C. Paladini, A. Jorissen +29

Our purpose is to study the effect of binary companions located within the first 10 stellar radii from the primary AGB star. In this work, we target the mass-losing carbon star V H…

astro-ph.SR2013

The H-band Emitting Region of the Luminous Blue Variable P Cygni: Spectrophotometry and Interferometry of the Wind

N. D. Richardson, G. H. Schaefer, D. R. Gies +20

We present the first high angular resolution observations in the nearinfrared H-band (1.6 microns) of the Luminous Blue Variable star P Cygni. We obtained six-telescope interferome…

astro-ph.SR2023

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.SR2018

A geometrical 1% distance to the short-period binary Cepheid V1334 Cygni

A. Gallenne, P. Kervella, N. R. Evans +18

Cepheid stars play a considerable role as extragalactic distances indicators, thanks to the simple empirical relation between their pulsation period and their luminosity. They over…

astro-ph.SR2020

A family portrait of disk inner rims around Herbig Ae/Be stars: Hunting for warps, rings, self shadowing, and misalignments in the inner astronomical units

J. Kluska, J. -P. Berger, F. Malbet +25

The innermost astronomical unit in protoplanetary disks is a key region for stellar and planet formation, as exoplanet searches have shown a large occurrence of close-in planets th…

astro-ph.SR2015

Robust high-contrast companion detection from interferometric observations. The CANDID algorithm and an application to six binary Cepheids

A. Gallenne, A. Mérand, P. Kervella +15

Long-baseline interferometry is an important technique to spatially resolve binary or multiple systems in close orbits. By combining several telescopes together and spectrally disp…

astro-ph.IM2012

Imaging the heart of astrophysical objects with optical long-baseline interferometry

J. -P. Berger, F. Malbet, F. Baron +21

The number of publications of aperture-synthesis images based on optical long-baseline interferometry measurements has recently increased due to easier access to visible and infrar…

astro-ph.SR2018

Multiplicity of Galactic Cepheids from long-baseline interferometry. IV. New detected companions from MIRC and PIONIER observations

A. Gallenne, P. Kervella, S. Borgniet +10

We aim at detecting and characterizing the main-sequence companions of a sample of known and suspected Galactic binary Cepheids. We used the multi-telescope interferometric combine…

astro-ph.SR2016

Structure of Herbig AeBe disks at the milliarcsecond scale A statistical survey in the H band using PIONIER-VLTI

B. Lazareff, J. -P. Berger, J. Kluska +26

Context. It is now generally accepted that the near-infrared excess of Herbig AeBe stars originates in the dust of a circumstellar disk. Aims. The aims of this article are to infer…

astro-ph.SR2014

CHARA/MIRC observations of two M supergiants in Perseus OB1: temperature, Bayesian modeling, and compressed sensing imaging

F. Baron, J. D. Monnier, L. L. Kiss +12

Two red supergiants of the Per OB1 association, RS Per and T Per, have been observed in H band using the MIRC instrument at the CHARA array. The data show clear evidence of departu…

astro-ph.SR2024

A new dimension in the variability of AGB stars: convection patterns size changes with pulsation

A. Rosales-Guzmán, J. Sanchez-Bermudez, C. Paladini +16

Stellar convection plays an important role in atmospheric dynamics, wind formation and the mass-loss processes in Asymptotic Giant Branch (AGB) stars. However, a direct characteriz…

astro-ph.IM2024

ANDES, the high resolution spectrograph for the ELT: science goals, project overview and future developments

A. Marconi, M. Abreu, V. Adibekyan +286

The first generation of ELT instruments includes an optical-infrared high-resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion E…

astro-ph.SR2013

Interferometric radii of bright Kepler stars with the CHARA Array: θ Cygni and 16 Cygni A and B

T. R. White, D. Huber, V. Maestro +18

We present the results of long-baseline optical interferometry observations using the Precision Astronomical Visual Observations (PAVO) beam combiner at the Center for High Angular…

astro-ph.IM2014

SPARCO : a semi-parametric approach for image reconstruction of chromatic objects

J. Kluska, F. Malbet, J. -P. Berger +6

The emergence of optical interferometers with three and more telescopes allows image reconstruction of astronomical objects at the milliarcsecond scale. However, some objects conta…

astro-ph.SR2015

Spectral and spatial imaging of the Be+sdO binary phi Persei

D. Mourard, J. D. Monnier, A. Meilland +25

The rapidly rotating Be star phi Persei was spun up by mass and angular momentum transfer from a now stripped-down, hot subdwarf companion. Here we present the first high angular r…

astro-ph.SR2015

First Images of Cool Starspots on a Star Other than the Sun: Interferometric Imaging of Andromedae

J. R. Parks, R. J. White, F. Baron +14

Presented are the first interferometric images of cool starspots on the chromospherically active giant Andromedae. These images represent the first model-independent images of…

astro-ph.SR2018

Physical properties of beta Lyr A and its opaque accretion disk

D. Mourard, M. Broz, J. Nemravova +23

Mass exchange and mass loss in close binaries can significantly affect their evolution, but a complete self-consistent theory of these processes is still to be developed. Processes…

astro-ph.SR2014

Multiplicity of Galactic Cepheids from long-baseline interferometry I. CHARA/MIRC detection of the companion of V1334 Cygni

A. Gallenne, J. D. Monnier, A. Mérand +16

We aim at determining the masses of Cepheids in binary systems, as well as their geometric distances and the flux contribution of the companions. The combination of interferometry…