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Dynamical Evidence of a Spiral Arm–driving Planet in the MWC 758 Protoplanetary Disk

Ren, Bin and Dong, Ruobing and van Holstein, Rob G. and Ruffio, Jean-Baptiste and Calvin, Benjamin A. and Girard, Julien H. and Benisty, Myriam and Boccaletti, Anthony and Esposito, Thomas M. and Choquet, Élodie and Mawet, Dimitri and Pueyo, Laurent and Stolker, Tomas and Chiang, Eugene and De Boer, Jozua and Debes, John H. and Garufi, Antonio and Grady, Carol A. and Hines, Dean C. and Maire, Anne-Lise and Ménard, François and Millar-Blanchaer, Maxwell A. and Perrin, Marshall D. and Poteet, Charles A. and Schneider, Glenn (2020) Dynamical Evidence of a Spiral Arm–driving Planet in the MWC 758 Protoplanetary Disk. Astrophysical Journal Letters, 898 (2). Art. No. L38. ISSN 2041-8213. https://resolver.caltech.edu/CaltechAUTHORS:20200729-095324179

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Abstract

More than a dozen young stars host spiral arms in their surrounding protoplanetary disks. The excitation mechanisms of such arms are under debate. The two leading hypotheses—companion–disk interaction and gravitational instability (GI)—predict distinct motion for spirals. By imaging the MWC 758 spiral arm system at two epochs spanning ~5 yr using the SPHERE instrument on the Very Large Telescope, we test the two hypotheses for the first time. We find that the pattern speeds of the spirals are not consistent with the GI origin. Our measurements further evince the existence of a faint "missing planet" driving the disk arms. The average spiral pattern speed is 0.°22 ± 0.°03 yr⁻¹, pointing to a driver at 172⁺¹⁸₋₁₄ au around a 1.9 M_☉ central star if it is on a circular orbit. In addition, we witness time-varying shadowing effects on a global scale that are likely originating from an inner disk.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/2041-8213/aba43eDOIArticle
https://arxiv.org/abs/2007.04980arXivDiscussion Paper
ORCID:
AuthorORCID
Ren, Bin0000-0003-1698-9696
Dong, Ruobing0000-0001-9290-7846
van Holstein, Rob G.0000-0003-1520-8405
Ruffio, Jean-Baptiste0000-0003-2233-4821
Girard, Julien H.0000-0001-8627-0404
Benisty, Myriam0000-0002-7695-7605
Boccaletti, Anthony0000-0001-9353-2724
Esposito, Thomas M.0000-0002-0792-3719
Choquet, Élodie0000-0002-9173-0740
Mawet, Dimitri0000-0002-8895-4735
Pueyo, Laurent0000-0003-3818-408X
Stolker, Tomas0000-0002-5823-3072
Chiang, Eugene0000-0002-6246-2310
De Boer, Jozua0000-0002-1028-7522
Debes, John H.0000-0002-1783-8817
Garufi, Antonio0000-0002-4266-0643
Hines, Dean C.0000-0003-4653-6161
Maire, Anne-Lise0000-0002-2591-4138
Ménard, François0000-0002-1637-7393
Millar-Blanchaer, Maxwell A.0000-0001-6205-9233
Perrin, Marshall D.0000-0002-3191-8151
Poteet, Charles A.0000-0003-4845-7483
Schneider, Glenn0000-0002-4511-5966
Additional Information:© 2020 The American Astronomical Society. Received 2020 May 8; revised 2020 July 8; accepted 2020 July 8; published 2020 July 29. We thank the anonymous referee for comments that improved the clarity of this Letter, and Cassandra Hall for useful discussions. Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programmes 060.A-9389(A) and 104.C-0472(A). B.R. thanks Christian Ginski for discussions on shadowing effects, Rémi Soummer for initiating the Archival Legacy Investigations of Circumstellar Environments (ALICE) project that set up the stage for R18 and this Letter. T.E. was supported in part by NASA Grants NNX15AD95G/NEXSS, NNX15AC89G, and NSF AST-1518332. A.L.M. acknowledges the financial support of the F.R.S.-FNRS through a postdoctoral researcher grant. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. Facilities: Very Large Telescope (SPHERE) - , Keck:II (NIRC2). - Software: diskmap (Stolker et al. 2016), IRDAP (van Holstein et al. 2017, 2020), scipy (Virtanen et al. 2020).
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
NASANNX15AD95G
NASANNX15AC89G
NSFAST-1518332
Fonds de la Recherche Scientifique (FNRS)UNSPECIFIED
W. M. Keck FoundationUNSPECIFIED
Subject Keywords:Protoplanetary disks ; Coronagraphic imaging ; Planetary system formation ; Orbital motion
Issue or Number:2
Classification Code:Unified Astronomy Thesaurus concepts: Protoplanetary disks (1300); Coronagraphic imaging (313); Planetary system formation (1257); Orbital motion (1179)
Record Number:CaltechAUTHORS:20200729-095324179
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200729-095324179
Official Citation:Bin Ren et al 2020 ApJL 898 L38
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104634
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:29 Jul 2020 18:08
Last Modified:29 Jul 2020 18:08

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