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Dive into the research topics where A. Meilland is active.

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Featured researches published by A. Meilland.


Astronomy and Astrophysics | 2007

First direct detection of a Keplerian rotating disk around the Be star

A. Meilland; P. Stee; Martin Vannier; F. Millour; A. Domiciano de Souza; Fabien Malbet; C. Martayan; Francesco Paresce; Romain G. Petrov; A. Richichi; A. Spang

Aims. We aim to study the geometry and kinematics of the disk around the Be star


Astronomy and Astrophysics | 2007

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Fabien Malbet; M. Benisty; W. J. de Wit; S. Kraus; A. Meilland; F. Millour; E. Tatulli; J.-P. Berger; O. Chesneau; Karl-Heinz Hofmann; Andrea Isella; A. Natta; Romain G. Petrov; Thomas Preibisch; P. Stee; L. Testi; G. Weigelt; P. Antonelli; Udo Beckmann; Y. Bresson; A. Chelli; G. Duvert; L. Glück; P. Kern; S. Lagarde; E. Le Coarer; Franco Lisi; K. Perraut; Sylvie Robbe-Dubois; A. Roussel

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Astronomy and Astrophysics | 2012

Arae using the VLTI/AMBER instrument.

A. Meilland; F. Millour; Samer Kanaan; P. Stee; Romain G. Petrov; Karl-Heinz Hofmann; A. Natta; K. Perraut

Arae as a function of wavelength, especially across the Br


Astronomy and Astrophysics | 2011

Disk and wind interaction in the young stellar object MWC 297 spatially resolved with VLTI/AMBER

O. Delaa; Ph. Stee; A. Meilland; J. Zorec; D. Mourard; Ph. Bério; D. Bonneau; O. Chesneau; J. M. Clausse; Pierre Cruzalèbes; K. Perraut; A. Marcotto; A. Roussel; A. Spang; H. McAlister; Theo A. ten Brummelaar; J. Sturmann; L. Sturmann; Neal J. Turner; C. Farrington; P. J. Goldfinger

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Astronomy and Astrophysics | 2011

First spectro-interferometric survey of Be stars - I. Observations and constraints on the disk geometry and kinematics

O. Chesneau; A. Meilland; D. P. K. Banerjee; J.-B. Le Bouquin; Harold A. McAlister; F. Millour; S. T. Ridgway; A. Spang; Theo A. ten Brummelaar; Markus Wittkowski; N. M. Ashok; M. Benisty; Jean-Philippe Berger; Tabetha S. Boyajian; Ch. Farrington; P. J. Goldfinger; A. Mérand; N. Nardetto; Romain G. Petrov; Th. Rivinius; Gail H. Schaefer; Y. Touhami; G. Zins

emission line. The main purpose of this paper is to answer the question about the nature of the disk rotation around Be stars. Methods. We use the VLTI/AMBER instrument operating in the K band which provides a gain by a factor 5 in spatial resolution compared to previous VLTI/MIDI observations. Moreover, it is possible to combine the high angular resolution provided with the (medium) spectral resolution of AMBER to study the kinematics of the inner part of the disk and to infer its rotation law. Results. We obtain for the first time the direct evidence that the disk is in keplerian rotation, answering a question that occurs since the discovery of the first Be star


Astronomy and Astrophysics | 2005

Kinematics and geometrical study of the Be stars 48 Persei and ψ Persei with the VEGA/CHARA interferometer

O. Chesneau; A. Meilland; T. Rivinius; P. Stee; S. Jankov; A. Domiciano de Souza; U. Graser; T. M. Herbst; E. Janot-Pacheco; Ralf S. Koehler; Christoph Leinert; S. Morel; Francesco Paresce; A. Richichi; Sylvie Robbe-Dubois

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Astronomy and Astrophysics | 2006

The 2011 outburst of the recurrent nova T Pyxidis. Evidence for a face-on bipolar ejection

A. Meilland; P. Stee; J. Zorec; Samer Kanaan

Cas by father Secchi in 1866. We also present the global geometry of the disk showing that it is compatible with a thin disk + polar enhanced winds modeled with the SIMECA code. We found that the disk around


Astronomy and Astrophysics | 2015

First VLTI/MIDI observations of a Be star: Alpha Arae

D. Mourard; John D. Monnier; A. Meilland; Douglas R. Gies; F. Millour; M. Benisty; Xiaozhou Che; Erika D. Grundstrom; R. Ligi; Gail H. Schaefer; Fabien Baron; Stefan Kraus; Ming Zhao; E Pedretti; Philippe Berio; J. M. Clausse; N. Nardetto; K. Perraut; A. Spang; P. Stee; Isabelle Tallon-Bosc; H. McAlister; Theo A. ten Brummelaar; S. T. Ridgway; J. Sturmann; L. Sturmann; Neal J. Turner; C. Farrington

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Astronomy and Astrophysics | 2014

Be stars: one ring to rule them all ?

O. Chesneau; A. Meilland; E. Chapellier; F. Millour; A. M. van Genderen; Yaël Nazé; Nathan Smith; A. Spang; Jonathan Smoker; L. Dessart; Samer Kanaan; Ph. Bendjoya; M. W. Feast; Jose H. Groh; A. Lobel; N. Nardetto; S. Otero; R. D. Oudmaijer; A. G. Tekola; Patricia A. Whitelock; C. Arcos; Michel Cure; Leonardo Vanzi

Arae is compatible with a dense equatorial matter confined in the central region whereas a polar wind is contributing along the rotational axis of the central star. Between these two regions the density must be low enough to reproduce the large visibility modulus (small extension) obtained for two of the four VLTI baselines. Moreover, we obtain that


Astronomy and Astrophysics | 2012

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

Ph. Stee; O. Delaa; John D. Monnier; A. Meilland; K. Perraut; D. Mourard; Xiao Che; Gail H. Schaefer; Ettore Pedretti; Myron A. Smith; R. Lopes de Oliveira; C. Motch; Gregory W. Henry; N. D. Richardson; K. S. Bjorkman; R. Bücke; E. Pollmann; J. Zorec; Douglas R. Gies; Theo A. ten Brummelaar; H. McAlister; Nils H. Turner; J. Sturmann; L. Sturmann; S. T. Ridgway

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F. Millour

Centre national de la recherche scientifique

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D. Mourard

Centre national de la recherche scientifique

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N. Nardetto

Centre national de la recherche scientifique

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O. Chesneau

Centre national de la recherche scientifique

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A. Spang

Centre national de la recherche scientifique

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J. M. Clausse

Centre national de la recherche scientifique

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P. Stee

Centre national de la recherche scientifique

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K. Perraut

Joseph Fourier University

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Romain G. Petrov

Centre national de la recherche scientifique

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Ph. Stee

Centre national de la recherche scientifique

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