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Author | dc.contributor.author | Cieza, Lucas A. | |
Author | dc.contributor.author | Ruíz-Rodríguez, Dary | |
Author | dc.contributor.author | Hales, Antonio | |
Author | dc.contributor.author | Casassus Montero, Simón | |
Author | dc.contributor.author | Pérez, Sebastian | |
Author | dc.contributor.author | Gonzalez-Ruilova, Camilo | |
Author | dc.contributor.author | Cánovas, Hector | |
Author | dc.contributor.author | Williams, Jonathan P. | |
Author | dc.contributor.author | Zurlo, Alice | |
Author | dc.contributor.author | Ansdell, Megan | |
Author | dc.contributor.author | Avenhaus, Henning | |
Author | dc.contributor.author | Bayo, Amelia | |
Author | dc.contributor.author | Bertrang, Gesa H.M. | |
Author | dc.contributor.author | Christiaens, Valentin | |
Author | dc.contributor.author | Dent, | |
Admission date | dc.date.accessioned | 2019-10-11T17:31:26Z | |
Available date | dc.date.available | 2019-10-11T17:31:26Z | |
Publication date | dc.date.issued | 2019 | |
Cita de ítem | dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, Volumen 482, Issue 1, 2019, Pages 698-714 | |
Identifier | dc.identifier.issn | 13652966 | |
Identifier | dc.identifier.issn | 00358711 | |
Identifier | dc.identifier.other | 10.1093/mnras/sty2653 | |
Identifier | dc.identifier.uri | https://repositorio.uchile.cl/handle/2250/171375 | |
Abstract | dc.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 | |
Lenguage | dc.language.iso | en | |
Publisher | dc.publisher | Oxford University Press | |
Type of license | dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Chile | |
Link to License | dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
Source | dc.source | Monthly Notices of the Royal Astronomical Society | |
Keywords | dc.subject | Circumstellar matter | |
Keywords | dc.subject | Protoplanetary discs | |
Keywords | dc.subject | Stars: pre-main-sequence | |
Keywords | dc.subject | Submillimetre: planetary systems | |
Título | dc.title | The Ophiuchus DIsc Survey Employing ALMA (ODISEA) - I: Project description and continuum images at 28 au resolution | |
Document type | dc.type | Artículo de revista | |
dcterms.accessRights | dcterms.accessRights | Acceso Abierto | |
Cataloguer | uchile.catalogador | SCOPUS | |
Indexation | uchile.index | Artículo de publicación SCOPUS | |
uchile.cosecha | uchile.cosecha | SI | |
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