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Authordc.contributor.authorThalmann, C. 
Authordc.contributor.authorMulders, G. D. 
Authordc.contributor.authorJanson, M. 
Authordc.contributor.authorOlofsson, J. 
Authordc.contributor.authorBenisty, Myriam 
Authordc.contributor.authorAvenhaus, H. 
Authordc.contributor.authorQuanz, S. P. 
Authordc.contributor.authorSchmid, H. M. 
Authordc.contributor.authorHenning, Thomas 
Authordc.contributor.authorBuenzli, E. 
Authordc.contributor.authorMénard, Francois 
Authordc.contributor.authorCarson, J. C. 
Authordc.contributor.authorGarufi, A. 
Authordc.contributor.authorMessina, S. 
Authordc.contributor.authorDominik, C. 
Authordc.contributor.authorLeisenring, J. 
Authordc.contributor.authorChauvin, G. 
Authordc.contributor.authorMeyer, M. R. 
Admission datedc.date.accessioned2015-10-30T15:32:44Z
Available datedc.date.available2015-10-30T15:32:44Z
Publication datedc.date.issued2015
Cita de ítemdc.identifier.citationThe Astrophysical Journal Letters, 808:L41 (7pp), 2015 August 1en_US
Identifierdc.identifier.otherdoi:10.1088/2041-8205/808/2/L41
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/134782
General notedc.descriptionArtículo de publicación ISIen_US
Abstractdc.description.abstractWe present the first optical (590-890 nm) imaging polarimetry observations of the pre-transitional protoplanetary disk around the young solar analog LkCa 15, addressing a number of open questions raised by previous studies. We detect the previously unseen far side of the disk gap, confirming the highly off-centered scattered-light gap shape that was postulated from near-infrared imaging, at odds with the symmetric gap inferred from millimeter interferometry. Furthermore, we resolve the inner disk for the first time and trace it out to 30 AU. This new source of scattered light may contribute to the near-infrared interferometric signal attributed to the protoplanet candidate LkCa 15 b, which lies embedded in the outer regions of the inner disk. Finally, we present a new model for the system architecture of LkCa 15 that ties these new findings together. These observations were taken during science verification of SPHERE ZIMPOL and demonstrate this facility's performance for faint guide stars under adverse observing conditions.en_US
Patrocinadordc.description.sponsorshipSwiss National Science Foundation SNSF European Commission under Marie Curie IEF 329875 Millennium Nucleus RC130007 NSF 1009203en_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherIOP Publishingen_US
Type of licensedc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectCircumstellar matteren_US
Keywordsdc.subjectPlanets and satellites: formationen_US
Keywordsdc.subjectProtoplanetary disksen_US
Keywordsdc.subjectStars: individual (LkCa 15)en_US
Keywordsdc.subjectStars: pre-main sequenceen_US
Keywordsdc.subjectTechniques: high angular resolutionen_US
Títulodc.titleOptical Imaging Polarimetry of the LkCa 15 protoplanetary Disk with Sphere Zimpolen_US
Document typedc.typeArtículo de revistaen_US


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Atribución-NoComercial-SinDerivadas 3.0 Chile
Except where otherwise noted, this item's license is described as Atribución-NoComercial-SinDerivadas 3.0 Chile