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Three-dimensional interferometric, spectrometric, and planetary views of Procyon

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Chiavassa, Andrea; Bigot, L; Kervella, Pierre; Matter, A; Lopez, B; Collet, Remo; Magic, Zazralt; Asplund, Martin

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Context. Procyon is one of the brightest stars in the sky and one of our nearest neighbours. It is therefore an ideal benchmark object for stellar astrophysics studies using interferometric, spectroscopic, and asteroseismic techniques. Aims. We use a new

dc.contributor.authorChiavassa, Andrea
dc.contributor.authorBigot, L
dc.contributor.authorKervella, Pierre
dc.contributor.authorMatter, A
dc.contributor.authorLopez, B
dc.contributor.authorCollet, Remo
dc.contributor.authorMagic, Zazralt
dc.contributor.authorAsplund, Martin
dc.date.accessioned2015-12-10T23:26:04Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/67612
dc.description.abstractContext. Procyon is one of the brightest stars in the sky and one of our nearest neighbours. It is therefore an ideal benchmark object for stellar astrophysics studies using interferometric, spectroscopic, and asteroseismic techniques. Aims. We use a new
dc.publisherSpringer
dc.rightsAuthor/s retain copyright
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: 3D simulations; Angular diameters; Bolometric flux; Circular symmetry; Closure phasis; Flux methods; Host-stars; Infrared filters; Intensity maps; Intensity profiles; Jupiters; Model atmosphere; Nearest neighbour; Photometric colors; planetary systems; Pr hydrodynamics; planetary systems; radiative transfer; stars: atmospheres; stars: individual: Procyon; techniques: interferometric
dc.titleThree-dimensional interferometric, spectrometric, and planetary views of Procyon
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume540
dc.date.issued2012
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB1487
local.identifier.ariespublicationu4630950xPUB61
local.type.statusPublished Version
local.contributor.affiliationChiavassa, Andrea, Universite Libre de Bruxelles
local.contributor.affiliationBigot, L, Université de Nice Sophia-Antipolis, Observatoire de la Côte d’Azur
local.contributor.affiliationKervella, Pierre, Observatoire de Paris
local.contributor.affiliationMatter, A, Max-Planck-Institut für Radioastronomie
local.contributor.affiliationLopez, B, Université de Nice Sophia-Antipolis, Observatoire de la Côte d’Azur
local.contributor.affiliationCollet, Remo, University of Copenhagen
local.contributor.affiliationMagic, Zazralt, Max-Planck-Institut für Astrophysik
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.bibliographicCitation.startpageA5
local.identifier.doi10.1051/0004-6361/201118652
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
dc.date.updated2016-02-24T08:47:14Z
local.identifier.scopusID2-s2.0-84858257885
local.identifier.thomsonID000303315400019
dcterms.accessRightsOpen Access
CollectionsANU Research Publications

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