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Authordc.contributor.authorMin, M. 
Authordc.contributor.authorStolker, T. 
Authordc.contributor.authorDominik, C. 
Authordc.contributor.authorBenisty, Myriam 
Admission datedc.date.accessioned2018-07-10T22:52:20Z
Available datedc.date.available2018-07-10T22:52:20Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationAstronomy & Astrophysics, 604, L10 (2017)es_ES
Identifierdc.identifier.other10.1051/0004-6361/201730949
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/149738
Abstractdc.description.abstractAims. Shadows in transitional disks are generally interpreted as signs of a misaligned inner disk. This disk is usually beyond the reach of current day high contrast imaging facilities. However, the location and morphology of the shadow features allow us to reconstruct the inner disk geometry. Methods. We derive analytic equations of the locations of the shadow features as a function of the orientation of the inner and outer disk and the height of the outer disk wall. In contrast to previous claims in the literature, we show that the position angle of the line connecting the shadows cannot be directly related to the position angle of the inner disk. Results. We show how the analytic framework derived here can be applied to transitional disks with shadow features. We use estimates of the outer disk height to put constraints on the inner disk orientation. In contrast with the results from Long et al. (2017, ApJ, 838, 62), we derive that for the disk surrounding HD 100453 the analytic estimates and interferometric observations result in a consistent picture of the orientation of the inner disk. Conclusions. The elegant consistency in our analytic framework between observation and theory strongly support both the interpretation of the shadow features as coming from a misaligned inner disk as well as the diagnostic value of near infrared interferometry for inner disk geometry.es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherEDP Scienceses_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceAstronomy & Astrophysicses_ES
Keywordsdc.subjectProtoplanetary diskses_ES
Keywordsdc.subjectTechniques interferometrices_ES
Keywordsdc.subjectTechniques high angular resolutiones_ES
Keywordsdc.subjectStars ariables: T Tauri, Herbig Ae/Bees_ES
Títulodc.titleConnecting the shadows: probing inner disk geometries using shadows in transitional diskses_ES
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadortjnes_ES
Indexationuchile.indexArtículo de publicación ISIes_ES


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile