Protoplanetary disks; 1300; Astrophysics - Earth and Planetary; Astrophysics; Astrophysics - Solar and Stellar Astrophysics
Abstract :
[en] Companions at subarcsecond separation from young stars are difficult to image. However, their presence can be inferred from the perturbations they create in the dust and gas of protoplanetary disks. Here we present a new interpretation of SPHERE polarized observations that reveal the previously detected inner spiral in the disk of HD 100546. The spiral coincides with a newly detected <SUP>12</SUP>CO inner spiral and the previously reported CO emission Doppler flip, which has been interpreted as the signature of an embedded protoplanet. Comparisons with hydrodynamical models indicate that this Doppler flip is instead the kinematic counterpart of the spiral, which is likely generated by an inner companion inside the disk cavity.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Norfolk, Brodie J.; ANU, Research School of Astronomy and Astrophysics
Pinte, Christophe; Monash University, School of Astrophysics, Institute de Planetologie et d'Astrophysique de Grenoble
Calcino, Josh; Los Alamos National Laboratory, Theoretical Division
Hammond, Iain; Monash University, School of Astrophysics
van der Marel, Nienke; Leiden Observatory
Price, Daniel J.; Monash University, School of Astrophysics
Maddison, Sarah T.; ANU, Research School of Astronomy and Astrophysics
Christiaens, Valentin ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Gonzalez, Jean-François; Observatoire de Lyon, Centre Recherche Astrophysique de Lyon
Blakely, Dori; University of Victoria, Canada
Rosotti, Giovanni; Leiden Observatory, University of Leicester, Department of Physics and Astronomy
Ginski, Christian; Leiden Observatory
Language :
English
Title :
The Origin of the Doppler Flip in HD 100546: A Large-scale Spiral Arm Generated by an Inner Binary Companion
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