Search Results - "Mérand, A."
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1
First Resolution of Microlensed Images
Published in The Astrophysical journal (20-01-2019)“…Abstract We employ Very Large Telescope Interferometer GRAVITY to resolve, for the first time, the two images generated by a gravitational microlens. The…”
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Colder and Hotter: Interferometric Imaging of β Cassiopeiae and α Leonis
Published in The Astrophysical journal (10-05-2011)Get full text
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Tracing a decade of activity towards a yellow hypergiant. The spectral and spatial morphology of IRC+10420 at au scales
Published in Monthly notices of the Royal Astronomical Society (02-08-2022)“…ABSTRACT The fate of a massive star during the latest stages of its evolution is highly dependent on its mass-loss history and geometry, with the yellow…”
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Imaging and Modeling Rapidly Rotating Stars: α Cephei and α Ophiuchi
Published in The Astrophysical journal (10-08-2009)Get full text
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A Geometrical 1% Distance to the Short-period Binary Cepheid V1334 Cygni
Published in The Astrophysical journal (10-11-2018)“…Cepheid stars play a considerable role as extragalactic distances indicators, thanks to the simple empirical relation between their pulsation period and their…”
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A magnetic massive star has experienced a stellar merger
Published in Science (American Association for the Advancement of Science) (12-04-2024)“…Massive stars (those ≥8 solar masses at formation) have radiative envelopes that cannot sustain a dynamo, the mechanism that produces magnetic fields in…”
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Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event
Published in The Astrophysical journal (01-07-2020)“…We report the lens mass and distance measurements of the nearby microlensing event TCP J05074264+2447555 (Kojima-1). We measure the microlens parallax vector…”
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First Results from the CHARA Array. IV. The Interferometric Radii of Low-Mass Stars
Published in The Astrophysical journal (10-06-2006)“…We have measured the angular diameters of six M dwarfs with the CHARA Array, a long-baseline optical interferometer located at Mount Wilson Observatory…”
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First Results from the CHARA Array. VII. Long-Baseline Interferometric Measurements of Vega Consistent with a Pole-On, Rapidly Rotating Star
Published in The Astrophysical journal (01-07-2006)“…We have obtained high-precision interferometric measurements of Vega with the CHARA Array and FLUOR beam combiner in the K' band at projected baselines between…”
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The Path Towards High-Contrast Imaging with the VLTI: The Hi-5 Project
Published in Experimental astronomy (01-12-2018)“…The development of high-contrast capabilities has long been recognized as one of the top priorities for the VLTI (Very Large Telescope Interferometer). As of…”
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CHARA Array K'-Band Measurements of the Angular Dimensions of Be Star Disks
Published in The Astrophysical journal (01-01-2007)“…We present the first K'-band, long-baseline interferometric observations of the northern Be stars g Cas, h Per, Tau, and Dra. The measurements were made with…”
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Multiplicity of Galactic Cepheids from long-baseline interferometry – III. Sub-percent limits on the relative brightness of a close companion of δ Cephei
Published in Monthly notices of the Royal Astronomical Society (11-09-2016)“…We report new CHARA/Michigan InfraRed Combiner interferometric observations of the Cepheid archetype δ Cep, which aimed at detecting the newly discovered…”
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Toward Direct Detection of Hot Jupiters with Precision Closure Phase: Calibration Studies and First Results from the CHARA Array
Published in Publications of the Astronomical Society of the Pacific (01-08-2011)“…Direct detection of thermal emission from nearby hot Jupiters has greatly advanced our knowledge of extrasolar planets in recent years. Since hot Jupiter…”
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Pre-main-sequence binaries with tidally disrupted discs: the Brγ in HD 104237
Published in Monthly notices of the Royal Astronomical Society (01-01-2013)“…Active pre-main-sequence binaries with separations of around 10 stellar radii present a wealth of phenomena unobserved in common systems. The study of these…”
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Multiplicity of Galactic Cepheids from long-baseline interferometry - III. Sub-percent limits on the relative brightness of a close companion of d Cephei
Published in Monthly notices of the Royal Astronomical Society (01-09-2016)“…We report new CHARA/Michigan InfraRed Combiner interferometric observations of the Cepheid archetype ... Cep, which aimed at detecting the newly discovered…”
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Four years’ interferometric observations of Galactic binary Cepheids
Published in EPJ Web of Conferences (01-01-2017)“…We give an update on our long-term program of Galactic Cepheids started in 2012, whose goal is to measure the visual orbits of Cepheid companions. Using the…”
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The cool brown dwarf Gliese 229 B is a close binary
Published in Nature (London) (31-10-2024)“…Owing to their similarities with giant exoplanets, brown dwarf companions of stars provide insights into the fundamental processes of planet formation and…”
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Gaia22dkvLb: A Microlensing Planet Potentially Accessible to Radial-velocity Characterization
Published in The Astronomical journal (01-08-2024)“…Abstract We report discovering an exoplanet from following up a microlensing event alerted by Gaia. The event Gaia22dkv is toward a disk source rather than the…”
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Submilliarcsecond Optical Interferometry of the High-mass X-Ray Binary BP Cru with VLTI/GRAVITY
Published in The Astrophysical journal (20-07-2017)“…We observe the high-mass X-ray binary (HMXB) BP Cru using interferometry in the near-infrared K band with VLTI/GRAVITY. Continuum visibilities are at most…”
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HD 181068: A Red Giant in a Triply Eclipsing Compact Hierarchical Triple System
Published in Science (American Association for the Advancement of Science) (08-04-2011)“…Hierarchical triple systems comprise a close binary and a more distant component. They are important for testing theories of star formation and of stellar…”
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