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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/41122
Ver los metadatos del registro completo
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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 Técnicas2025-10-22T11:09:25Zoai: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:34982025-10-22 11:09:25.712CONICET 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 |
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article |
| status_str |
publishedVersion |
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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 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
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IOP Publishing |
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IOP Publishing |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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