Show simple item record

Authordc.contributor.authorCieza, Lucas A. 
Authordc.contributor.authorRuíz-Rodríguez, Dary 
Authordc.contributor.authorHales, Antonio 
Authordc.contributor.authorCasassus Montero, Simón 
Authordc.contributor.authorPérez, Sebastian 
Authordc.contributor.authorGonzalez-Ruilova, Camilo 
Authordc.contributor.authorCánovas, Hector 
Authordc.contributor.authorWilliams, Jonathan P. 
Authordc.contributor.authorZurlo, Alice 
Authordc.contributor.authorAnsdell, Megan 
Authordc.contributor.authorAvenhaus, Henning 
Authordc.contributor.authorBayo, Amelia 
Authordc.contributor.authorBertrang, Gesa H.M. 
Authordc.contributor.authorChristiaens, Valentin 
Authordc.contributor.authorDent, 
Admission datedc.date.accessioned2019-10-11T17:31:26Z
Available datedc.date.available2019-10-11T17:31:26Z
Publication datedc.date.issued2019
Cita de ítemdc.identifier.citationMonthly Notices of the Royal Astronomical Society, Volumen 482, Issue 1, 2019, Pages 698-714
Identifierdc.identifier.issn13652966
Identifierdc.identifier.issn00358711
Identifierdc.identifier.other10.1093/mnras/sty2653
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/171375
Abstractdc.description.abstract© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project aiming to study the entire population of Spitzer-selected protoplanetary discs in theOphiuchus Molecular Cloud (~300 objects) from both millimetre continuum and CO isotopologues data. Here we present 1.3 mm/230 GHz continuum images of 147 targets at 0.2 arcsec (28 au) resolution and a typical rms of 0.15 mJy.We detect a total of 133 discs, including the individual components of 11 binary systems and 1 triple system. 60 of these discs are spatially resolved. We find clear substructures (inner cavities, rings, gaps, and/or spiral arms) in eight of the sources and hints of such structures in another four discs.We construct the disc luminosity function for our targets and perform preliminary comparisons to other regions. A simple conversion between flux and dust mass (adopting standard assumptions) indicates that a
Lenguagedc.language.isoen
Publisherdc.publisherOxford University Press
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourceMonthly Notices of the Royal Astronomical Society
Keywordsdc.subjectCircumstellar matter
Keywordsdc.subjectProtoplanetary discs
Keywordsdc.subjectStars: pre-main-sequence
Keywordsdc.subjectSubmillimetre: planetary systems
Títulodc.titleThe Ophiuchus DIsc Survey Employing ALMA (ODISEA) - I: Project description and continuum images at 28 au resolution
Document typedc.typeArtículo de revista
dcterms.accessRightsdcterms.accessRightsAcceso Abierto
Catalogueruchile.catalogadorSCOPUS
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


Files in this item

Icon

This item appears in the following Collection(s)

Show simple item record

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