The Disk Substructures at High Angular Resolution Project (DSHARP). IV. Characterizing Substructures and Interactions in Disks around Multiple Star Systems

To characterize the substructures induced in protoplanetary disks by the interaction between stars in multiple systems, we study the 1.25 mm continuum and the 12CO(J = 2-1) spectral line emission of the triple systems HT Lup and AS 205, at scales of 5 au, as part of the "Disk Substructures at H...

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Veröffentlicht in:	Astrophysical journal. Letters 2018-12, Vol.869 (2), p.L44
Hauptverfasser:	Kurtovic, Nicolás T., Pérez, Laura M., Benisty, Myriam, Zhu, Zhaohuan, Zhang, Shangjia, Huang, Jane, Andrews, Sean M., Dullemond, Cornelis P., Isella, Andrea, Bai, Xue-Ning, Carpenter, John M., Guzmán, Viviana V., Ricci, Luca, Wilner, David J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Angular resolution binaries (including multiple): close Continuum radiation Counter rotation Diameters dust, extinction Forecasting Kinematics Line spectra Misalignment Pitch (inclination) Planet formation Protoplanetary disks Protoplanets Rotating disks Sciences of the Universe Stellar systems Substructures techniques: high angular resolution
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