The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk

Spatially resolved structures in protoplanetary disks hint at unseen planets. Previous imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a ring-like outer disk, emission clumps, and spiral arms, all possibly generated by companions. We present ALMA dust continuum...

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Main Authors: Ruobing Dong, Sheng-yuan Liu, Josh Eisner, Sean Andrews, Jeffrey Fung, Zhaohuan Zhu, Eugene Chiang, Jun Hashimoto, Hauyu Baobab Liu, Simon Casassus, Thomas Esposito, Yasuhiro Hasegawa, Takayuki Muto, Yaroslav Pavlyuchenkov, David Wilner, Eiji Akiyama, Motohide Tamura, John Wisniewski
Format: Article
Language:English
Published: IOP Publishing 2018-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/aac6cb
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author Ruobing Dong
Sheng-yuan Liu
Josh Eisner
Sean Andrews
Jeffrey Fung
Zhaohuan Zhu
Eugene Chiang
Jun Hashimoto
Hauyu Baobab Liu
Simon Casassus
Thomas Esposito
Yasuhiro Hasegawa
Takayuki Muto
Yaroslav Pavlyuchenkov
David Wilner
Eiji Akiyama
Motohide Tamura
John Wisniewski
author_facet Ruobing Dong
Sheng-yuan Liu
Josh Eisner
Sean Andrews
Jeffrey Fung
Zhaohuan Zhu
Eugene Chiang
Jun Hashimoto
Hauyu Baobab Liu
Simon Casassus
Thomas Esposito
Yasuhiro Hasegawa
Takayuki Muto
Yaroslav Pavlyuchenkov
David Wilner
Eiji Akiyama
Motohide Tamura
John Wisniewski
author_sort Ruobing Dong
collection DOAJ
description Spatially resolved structures in protoplanetary disks hint at unseen planets. Previous imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a ring-like outer disk, emission clumps, and spiral arms, all possibly generated by companions. We present ALMA dust continuum observations of MWC 758 at 0.87 mm wavelength with 43 × 39 mas angular resolution (6.9 × 6.2 au) and 20 μ Jy beam ^−1 rms. The central submillimeter emission cavity is revealed to be eccentric; once deprojected, its outer edge can be well fitted by an ellipse with an eccentricity of 0.1 and one focus on the star. The broad ring-like outer disk is resolved into three narrow rings with two gaps in between. The outer two rings tentatively show the same eccentricity and orientation as the innermost ring bounding the inner cavity. The two previously known dust emission clumps are resolved in both the radial and azimuthal directions, with radial widths equal to ∼4× the local scale height. Only one of the two spiral arms previously imaged in near-infrared (NIR) scattered light is revealed in ALMA dust emission, at a slightly larger stellocentric distance owing to projection effects. We also submit evidence of disk truncation at ∼100 au based on comparing NIR imaging observations with models. The spirals, the north clump, and the truncated disk edge are all broadly consistent with the presence of one companion exterior to the spirals at roughly 100 au.
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spelling doaj.art-5386f69c59a04fdcb39cda1ff5fa0b092023-10-11T14:25:01ZengIOP PublishingThe Astrophysical Journal1538-43572018-01-01860212410.3847/1538-4357/aac6cbThe Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 DiskRuobing Dong0https://orcid.org/0000-0001-9290-7846Sheng-yuan Liu1Josh Eisner2https://orcid.org/0000-0002-1031-4199Sean Andrews3https://orcid.org/0000-0003-2253-2270Jeffrey Fung4Zhaohuan Zhu5Eugene Chiang6https://orcid.org/0000-0002-6246-2310Jun Hashimoto7Hauyu Baobab Liu8Simon Casassus9https://orcid.org/0000-0002-0433-9840Thomas Esposito10https://orcid.org/0000-0002-0792-3719Yasuhiro Hasegawa11Takayuki Muto12Yaroslav Pavlyuchenkov13David Wilner14https://orcid.org/0000-0003-1526-7587Eiji Akiyama15https://orcid.org/0000-0002-5082-8880Motohide Tamura16https://orcid.org/0000-0002-6510-0681John Wisniewski17https://orcid.org/0000-0001-9209-1808Steward Observatory, University of Arizona , Tucson, AZ 85721, USA; Institute of Astronomy and Astrophysics , Academia Sinica, Taipei 10617, Taiwan, Republic of ChinaInstitute of Astronomy and Astrophysics , Academia Sinica, Taipei 10617, Taiwan, Republic of ChinaSteward Observatory, University of Arizona , Tucson, AZ 85721, USAHarvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USADepartment of Astronomy, University of California at Berkeley , Campbell Hall, Berkeley, CA 94720-3411, USADepartment of Physics and Astronomy, University of Nevada , Las Vegas, 4505 South Maryland Parkway, Las Vegas, NV 89154, USADepartment of Astronomy, University of California at Berkeley , Campbell Hall, Berkeley, CA 94720-3411, USAAstrobiology Center of NINS, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, JapanEuropean Southern Observatory (ESO), Karl-Schwarzschild-Str. 2, D-85748 Garching, GermanyDepartamento de Astronomia, Universidad de Chile , Casilla 36-D, Santiago, ChileDepartment of Astronomy, University of California at Berkeley , Campbell Hall, Berkeley, CA 94720-3411, USAJet Propulsion Laboratory, California Institute of Technology , Pasadena, CA 91109, USADivision of Liberal Arts, Kogakuin University , 1-24-2 Nishi-Shinjuku, Shinjuku-ku, Tokyo 163-8677, JapanInstitute of Astronomy , Russian Academy of Sciences, Moscow, RussiaHarvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USANational Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JapanAstrobiology Center of NINS, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan; Department of Astronomy, The University of Tokyo , 7-3-1, Hongo, Bunkyo-ku, Tokyo 113-0033, JapanH. L. Dodge Department of Physics & Astronomy, University of Oklahoma , 440 W. Brooks St., Norman, OK 73019, USASpatially resolved structures in protoplanetary disks hint at unseen planets. Previous imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a ring-like outer disk, emission clumps, and spiral arms, all possibly generated by companions. We present ALMA dust continuum observations of MWC 758 at 0.87 mm wavelength with 43 × 39 mas angular resolution (6.9 × 6.2 au) and 20 μ Jy beam ^−1 rms. The central submillimeter emission cavity is revealed to be eccentric; once deprojected, its outer edge can be well fitted by an ellipse with an eccentricity of 0.1 and one focus on the star. The broad ring-like outer disk is resolved into three narrow rings with two gaps in between. The outer two rings tentatively show the same eccentricity and orientation as the innermost ring bounding the inner cavity. The two previously known dust emission clumps are resolved in both the radial and azimuthal directions, with radial widths equal to ∼4× the local scale height. Only one of the two spiral arms previously imaged in near-infrared (NIR) scattered light is revealed in ALMA dust emission, at a slightly larger stellocentric distance owing to projection effects. We also submit evidence of disk truncation at ∼100 au based on comparing NIR imaging observations with models. The spirals, the north clump, and the truncated disk edge are all broadly consistent with the presence of one companion exterior to the spirals at roughly 100 au.https://doi.org/10.3847/1538-4357/aac6cbplanet–disk interactionsplanets and satellites: formationprotoplanetary disksstars: individual (MWC 758)stars: variables: T Tauri, Herbig Ae/Be
spellingShingle Ruobing Dong
Sheng-yuan Liu
Josh Eisner
Sean Andrews
Jeffrey Fung
Zhaohuan Zhu
Eugene Chiang
Jun Hashimoto
Hauyu Baobab Liu
Simon Casassus
Thomas Esposito
Yasuhiro Hasegawa
Takayuki Muto
Yaroslav Pavlyuchenkov
David Wilner
Eiji Akiyama
Motohide Tamura
John Wisniewski
The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk
The Astrophysical Journal
planet–disk interactions
planets and satellites: formation
protoplanetary disks
stars: individual (MWC 758)
stars: variables: T Tauri, Herbig Ae/Be
title The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk
title_full The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk
title_fullStr The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk
title_full_unstemmed The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk
title_short The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk
title_sort eccentric cavity triple rings two armed spirals and double clumps of the mwc 758 disk
topic planet–disk interactions
planets and satellites: formation
protoplanetary disks
stars: individual (MWC 758)
stars: variables: T Tauri, Herbig Ae/Be
url https://doi.org/10.3847/1538-4357/aac6cb
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