ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud

Autores
Cieza, Lucas A.; Casassus, Simon; Pérez, Sebastian; Hales, Antonio; Cárcamo, Miguel; Ansdell, Megan; Avenhaus, Henning; Bayo, Amelia; Bertrang, Gesa H.-M.; Cánovas, Hector; Christiaens, Valentin; Dent, William; Ferrero, Gabriel; Gamen, Roberto Claudio; Olofsson, Johan; Orcajo, Santiago; Osses, Axel; Peña Ramirez, Karla; Principe, David; Ruíz Rodríguez, Dary; Schreiber, Matthias R.; Plas, Gerrit van der; Williams, Jonathan P.; Zurlo, Alice
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present ALMA 1.3 mm continuum observations at 0. 2 (25 au) resolution of Elias 2–24, one of the largest and brightest protoplanetary disks in the Ophiuchus Molecular Cloud, and we report the presence of three partially resolved concentric gaps located at ∼20, 52, and 87 au from the star. We perform radiative transfer modeling of the disk to constrain its surface density and temperature radial profile and place the disk structure in the context of mechanisms capable of forming narrow gaps such as condensation fronts and dynamical clearing by actively forming planets. In particular, we estimate the disk temperature at the locations of the gaps to be 23, 15, and 12 K (at 20, 52, and 87 au, respectively), very close to the expected snowlines of CO (23–28 K) and N2 (12–15 K). Similarly, by assuming that the widths of the gaps correspond to 4–8× the Hill radii of forming planets (as suggested by numerical simulations), we estimate planet masses in the range of 0.2 1.5 – MJup, 1.0 8.0 – MJup, and 0.02 0.15 – MJup for the inner, middle, and outer gap, respectively. Given the surface density profile of the disk, the amount of “missing mass” at the location of each one of these gaps (between 4 and 20 MJup) is more than sufficient to account for the formation of such planets.
Fil: Cieza, Lucas A.. Universidad Diego Portales; Chile
Fil: Casassus, Simon. Universidad de Chile; Chile
Fil: Pérez, Sebastian. Universidad de Chile; Chile
Fil: Hales, Antonio. Alma Observatory; Chile
Fil: Cárcamo, Miguel. Universidad de Chile; Chile
Fil: Ansdell, Megan. University of California at Berkeley; Estados Unidos
Fil: Avenhaus, Henning. Universitat Zurich; Suiza
Fil: Bayo, Amelia. Universidad de Valparaiso; Chile
Fil: Bertrang, Gesa H.-M.. Universidad Diego Portales; Chile
Fil: Cánovas, Hector. Agencia Espacial Europea; España
Fil: Christiaens, Valentin. Universidad de Chile; Chile
Fil: Dent, William. Alma Observatory; Chile
Fil: Ferrero, Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Gamen, Roberto Claudio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Olofsson, Johan. Universidad de Valparaiso; Chile
Fil: Orcajo, Santiago. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Osses, Axel. Universidad de Chile; Chile
Fil: Peña Ramirez, Karla. Universidad de Antofagasta; Chile
Fil: Principe, David. Massachusetts Institute of Technology; Estados Unidos
Fil: Ruíz Rodríguez, Dary. Rochester Institute Of Technology; Estados Unidos
Fil: Schreiber, Matthias R.. Universidad de Valparaiso; Chile
Fil: Plas, Gerrit van der. Univ. Grenoble Alpes; Suiza
Fil: Williams, Jonathan P.. Institute For Astronomy, University Of Hawaii; Estados Unidos
Fil: Zurlo, Alice. Universidad Diego Portales; Chile
Materia
Circumstellar Matter
Planetary Systems
Protoplanetary Disks
Elias 2-24 (Estrella)
Interferometric Techniques
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/41122

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oai_identifier_str oai:ri.conicet.gov.ar:11336/41122
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloudCieza, Lucas A.Casassus, SimonPérez, SebastianHales, AntonioCárcamo, MiguelAnsdell, MeganAvenhaus, HenningBayo, AmeliaBertrang, Gesa H.-M.Cánovas, HectorChristiaens, ValentinDent, WilliamFerrero, GabrielGamen, Roberto ClaudioOlofsson, JohanOrcajo, SantiagoOsses, AxelPeña Ramirez, KarlaPrincipe, DavidRuíz Rodríguez, DarySchreiber, Matthias R.Plas, Gerrit van derWilliams, Jonathan P.Zurlo, AliceCircumstellar MatterPlanetary SystemsProtoplanetary DisksElias 2-24 (Estrella)Interferometric Techniqueshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present ALMA 1.3 mm continuum observations at 0. 2 (25 au) resolution of Elias 2–24, one of the largest and brightest protoplanetary disks in the Ophiuchus Molecular Cloud, and we report the presence of three partially resolved concentric gaps located at ∼20, 52, and 87 au from the star. We perform radiative transfer modeling of the disk to constrain its surface density and temperature radial profile and place the disk structure in the context of mechanisms capable of forming narrow gaps such as condensation fronts and dynamical clearing by actively forming planets. In particular, we estimate the disk temperature at the locations of the gaps to be 23, 15, and 12 K (at 20, 52, and 87 au, respectively), very close to the expected snowlines of CO (23–28 K) and N2 (12–15 K). Similarly, by assuming that the widths of the gaps correspond to 4–8× the Hill radii of forming planets (as suggested by numerical simulations), we estimate planet masses in the range of 0.2 1.5 – MJup, 1.0 8.0 – MJup, and 0.02 0.15 – MJup for the inner, middle, and outer gap, respectively. Given the surface density profile of the disk, the amount of “missing mass” at the location of each one of these gaps (between 4 and 20 MJup) is more than sufficient to account for the formation of such planets.Fil: Cieza, Lucas A.. Universidad Diego Portales; ChileFil: Casassus, Simon. Universidad de Chile; ChileFil: Pérez, Sebastian. Universidad de Chile; ChileFil: Hales, Antonio. Alma Observatory; ChileFil: Cárcamo, Miguel. Universidad de Chile; ChileFil: Ansdell, Megan. University of California at Berkeley; Estados UnidosFil: Avenhaus, Henning. Universitat Zurich; SuizaFil: Bayo, Amelia. Universidad de Valparaiso; ChileFil: Bertrang, Gesa H.-M.. Universidad Diego Portales; ChileFil: Cánovas, Hector. Agencia Espacial Europea; EspañaFil: Christiaens, Valentin. Universidad de Chile; ChileFil: Dent, William. Alma Observatory; ChileFil: Ferrero, Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Gamen, Roberto Claudio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Olofsson, Johan. Universidad de Valparaiso; ChileFil: Orcajo, Santiago. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Osses, Axel. Universidad de Chile; ChileFil: Peña Ramirez, Karla. Universidad de Antofagasta; ChileFil: Principe, David. Massachusetts Institute of Technology; Estados UnidosFil: Ruíz Rodríguez, Dary. Rochester Institute Of Technology; Estados UnidosFil: Schreiber, Matthias R.. Universidad de Valparaiso; ChileFil: Plas, Gerrit van der. Univ. Grenoble Alpes; SuizaFil: Williams, Jonathan P.. Institute For Astronomy, University Of Hawaii; Estados UnidosFil: Zurlo, Alice. Universidad Diego Portales; ChileIOP Publishing2017-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/41122Cieza, Lucas A.; Casassus, Simon; Pérez, Sebastian; Hales, Antonio; Cárcamo, Miguel; et al.; ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud; IOP Publishing; Astrophysical Journal Letters; 851; 2; 12-2017; 23-292041-8213CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://stacks.iop.org/2041-8205/851/i=2/a=L23?key=crossref.8dbbff4f288ad0ab8e744aae79813b34info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/aa9b7binfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:40:46Zoai:ri.conicet.gov.ar:11336/41122instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:40:46.889CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
title ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
spellingShingle ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
Cieza, Lucas A.
Circumstellar Matter
Planetary Systems
Protoplanetary Disks
Elias 2-24 (Estrella)
Interferometric Techniques
title_short ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
title_full ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
title_fullStr ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
title_full_unstemmed ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
title_sort ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud
dc.creator.none.fl_str_mv Cieza, Lucas A.
Casassus, Simon
Pérez, Sebastian
Hales, Antonio
Cárcamo, Miguel
Ansdell, Megan
Avenhaus, Henning
Bayo, Amelia
Bertrang, Gesa H.-M.
Cánovas, Hector
Christiaens, Valentin
Dent, William
Ferrero, Gabriel
Gamen, Roberto Claudio
Olofsson, Johan
Orcajo, Santiago
Osses, Axel
Peña Ramirez, Karla
Principe, David
Ruíz Rodríguez, Dary
Schreiber, Matthias R.
Plas, Gerrit van der
Williams, Jonathan P.
Zurlo, Alice
author Cieza, Lucas A.
author_facet Cieza, Lucas A.
Casassus, Simon
Pérez, Sebastian
Hales, Antonio
Cárcamo, Miguel
Ansdell, Megan
Avenhaus, Henning
Bayo, Amelia
Bertrang, Gesa H.-M.
Cánovas, Hector
Christiaens, Valentin
Dent, William
Ferrero, Gabriel
Gamen, Roberto Claudio
Olofsson, Johan
Orcajo, Santiago
Osses, Axel
Peña Ramirez, Karla
Principe, David
Ruíz Rodríguez, Dary
Schreiber, Matthias R.
Plas, Gerrit van der
Williams, Jonathan P.
Zurlo, Alice
author_role author
author2 Casassus, Simon
Pérez, Sebastian
Hales, Antonio
Cárcamo, Miguel
Ansdell, Megan
Avenhaus, Henning
Bayo, Amelia
Bertrang, Gesa H.-M.
Cánovas, Hector
Christiaens, Valentin
Dent, William
Ferrero, Gabriel
Gamen, Roberto Claudio
Olofsson, Johan
Orcajo, Santiago
Osses, Axel
Peña Ramirez, Karla
Principe, David
Ruíz Rodríguez, Dary
Schreiber, Matthias R.
Plas, Gerrit van der
Williams, Jonathan P.
Zurlo, Alice
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Circumstellar Matter
Planetary Systems
Protoplanetary Disks
Elias 2-24 (Estrella)
Interferometric Techniques
topic Circumstellar Matter
Planetary Systems
Protoplanetary Disks
Elias 2-24 (Estrella)
Interferometric Techniques
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present ALMA 1.3 mm continuum observations at 0. 2 (25 au) resolution of Elias 2–24, one of the largest and brightest protoplanetary disks in the Ophiuchus Molecular Cloud, and we report the presence of three partially resolved concentric gaps located at ∼20, 52, and 87 au from the star. We perform radiative transfer modeling of the disk to constrain its surface density and temperature radial profile and place the disk structure in the context of mechanisms capable of forming narrow gaps such as condensation fronts and dynamical clearing by actively forming planets. In particular, we estimate the disk temperature at the locations of the gaps to be 23, 15, and 12 K (at 20, 52, and 87 au, respectively), very close to the expected snowlines of CO (23–28 K) and N2 (12–15 K). Similarly, by assuming that the widths of the gaps correspond to 4–8× the Hill radii of forming planets (as suggested by numerical simulations), we estimate planet masses in the range of 0.2 1.5 – MJup, 1.0 8.0 – MJup, and 0.02 0.15 – MJup for the inner, middle, and outer gap, respectively. Given the surface density profile of the disk, the amount of “missing mass” at the location of each one of these gaps (between 4 and 20 MJup) is more than sufficient to account for the formation of such planets.
Fil: Cieza, Lucas A.. Universidad Diego Portales; Chile
Fil: Casassus, Simon. Universidad de Chile; Chile
Fil: Pérez, Sebastian. Universidad de Chile; Chile
Fil: Hales, Antonio. Alma Observatory; Chile
Fil: Cárcamo, Miguel. Universidad de Chile; Chile
Fil: Ansdell, Megan. University of California at Berkeley; Estados Unidos
Fil: Avenhaus, Henning. Universitat Zurich; Suiza
Fil: Bayo, Amelia. Universidad de Valparaiso; Chile
Fil: Bertrang, Gesa H.-M.. Universidad Diego Portales; Chile
Fil: Cánovas, Hector. Agencia Espacial Europea; España
Fil: Christiaens, Valentin. Universidad de Chile; Chile
Fil: Dent, William. Alma Observatory; Chile
Fil: Ferrero, Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Gamen, Roberto Claudio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Olofsson, Johan. Universidad de Valparaiso; Chile
Fil: Orcajo, Santiago. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Osses, Axel. Universidad de Chile; Chile
Fil: Peña Ramirez, Karla. Universidad de Antofagasta; Chile
Fil: Principe, David. Massachusetts Institute of Technology; Estados Unidos
Fil: Ruíz Rodríguez, Dary. Rochester Institute Of Technology; Estados Unidos
Fil: Schreiber, Matthias R.. Universidad de Valparaiso; Chile
Fil: Plas, Gerrit van der. Univ. Grenoble Alpes; Suiza
Fil: Williams, Jonathan P.. Institute For Astronomy, University Of Hawaii; Estados Unidos
Fil: Zurlo, Alice. Universidad Diego Portales; Chile
description We present ALMA 1.3 mm continuum observations at 0. 2 (25 au) resolution of Elias 2–24, one of the largest and brightest protoplanetary disks in the Ophiuchus Molecular Cloud, and we report the presence of three partially resolved concentric gaps located at ∼20, 52, and 87 au from the star. We perform radiative transfer modeling of the disk to constrain its surface density and temperature radial profile and place the disk structure in the context of mechanisms capable of forming narrow gaps such as condensation fronts and dynamical clearing by actively forming planets. In particular, we estimate the disk temperature at the locations of the gaps to be 23, 15, and 12 K (at 20, 52, and 87 au, respectively), very close to the expected snowlines of CO (23–28 K) and N2 (12–15 K). Similarly, by assuming that the widths of the gaps correspond to 4–8× the Hill radii of forming planets (as suggested by numerical simulations), we estimate planet masses in the range of 0.2 1.5 – MJup, 1.0 8.0 – MJup, and 0.02 0.15 – MJup for the inner, middle, and outer gap, respectively. Given the surface density profile of the disk, the amount of “missing mass” at the location of each one of these gaps (between 4 and 20 MJup) is more than sufficient to account for the formation of such planets.
publishDate 2017
dc.date.none.fl_str_mv 2017-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/41122
Cieza, Lucas A.; Casassus, Simon; Pérez, Sebastian; Hales, Antonio; Cárcamo, Miguel; et al.; ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud; IOP Publishing; Astrophysical Journal Letters; 851; 2; 12-2017; 23-29
2041-8213
CONICET Digital
CONICET
url http://hdl.handle.net/11336/41122
identifier_str_mv Cieza, Lucas A.; Casassus, Simon; Pérez, Sebastian; Hales, Antonio; Cárcamo, Miguel; et al.; ALMA observations of Elias 2–24: a protoplanetary disk with multiple gaps in the Ophiuchus molecular cloud; IOP Publishing; Astrophysical Journal Letters; 851; 2; 12-2017; 23-29
2041-8213
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://stacks.iop.org/2041-8205/851/i=2/a=L23?key=crossref.8dbbff4f288ad0ab8e744aae79813b34
info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8213/aa9b7b
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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