A Magnetically Driven Disk Wind in the Inner Disk of PDS 70*

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dc.citation.articleNumber25en_US
dc.citation.issueNumber1en_US
dc.citation.journalTitleThe Astrophysical Journalen_US
dc.citation.volumeNumber956en_US
dc.contributor.authorCampbell-White, Justynen_US
dc.contributor.authorManara, Carlo F.en_US
dc.contributor.authorBenisty, Myriamen_US
dc.contributor.authorNatta, Antonellaen_US
dc.contributor.authorClaes, Rik A. B.en_US
dc.contributor.authorFrasca, Antonioen_US
dc.contributor.authorBae, Jaehanen_US
dc.contributor.authorFacchini, Stefanoen_US
dc.contributor.authorIsella, Andreaen_US
dc.contributor.authorPérez, Lauraen_US
dc.contributor.authorPinilla, Paolaen_US
dc.contributor.authorSicilia-Aguilar, Auroraen_US
dc.contributor.authorTeague, Richarden_US
dc.date.accessioned2024-05-08T18:56:11Zen_US
dc.date.available2024-05-08T18:56:11Zen_US
dc.date.issued2023en_US
dc.description.abstractPDS 70 is so far the only young disk where multiple planets have been detected by direct imaging. The disk has a large cavity when seen at submillimeter and near-infrared wavelengths, which hosts two massive planets. This makes PDS 70 the ideal target to study the physical conditions in a strongly depleted inner disk shaped by two giant planets, and in particular to test whether disk winds can play a significant role in its evolution. Using X-Shooter and HARPS spectra, we detected for the first time the wind-tracing [O i] 6300 Å line, and confirm the low-moderate value of mass-accretion rate in the literature. The [O i] line luminosity is high with respect to the accretion luminosity when compared to a large sample of disks with cavities in nearby star-forming regions. The FWHM and blueshifted peak of the [O i] line suggest an emission in a region very close to the star, favoring a magnetically driven wind as the origin. We also detect wind emission and high variability in the He i 10830 Å line, which is unusual for low accretors. We discuss that, although the cavity of PDS 70 was clearly carved out by the giant planets, the substantial inner-disk wind could also have had a significant contribution to clearing the inner disk.en_US
dc.identifier.citationCampbell-White, J., Manara, C. F., Benisty, M., Natta, A., Claes, R. A. B., Frasca, A., Bae, J., Facchini, S., Isella, A., Pérez, L., Pinilla, P., Sicilia-Aguilar, A., & Teague, R. (2023). A Magnetically Driven Disk Wind in the Inner Disk of PDS 70*. The Astrophysical Journal, 956(1), 25. https://doi.org/10.3847/1538-4357/acf0c0en_US
dc.identifier.digitalCampbell-White_2023_ApJ_956_25en_US
dc.identifier.doihttps://doi.org/10.3847/1538-4357/acf0c0en_US
dc.identifier.urihttps://hdl.handle.net/1911/115679en_US
dc.language.isoengen_US
dc.publisherIOP Publishing Ltden_US
dc.rightsExcept where otherwise noted, this work is licensed under a Creative Commons Attribution (CC BY) license. Permission to reuse, publish, or reproduce the work beyond the terms of the license or beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleA Magnetically Driven Disk Wind in the Inner Disk of PDS 70*en_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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