1. External or internal companion exciting the spiral arms in CQ Tau?
- Author
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Hammond, Iain, Christiaens, Valentin, Price, Daniel J, Ubeira-Gabellini, Maria Giulia, Baird, Jennifer, Calcino, Josh, Benisty, Myriam, Lodato, Giuseppe, Testi, Leonardo, Pinte, Christophe, Toci, Claudia, and Fedele, Davide
- Subjects
PROTOPLANETARY disks ,GAS giants ,ORBITS (Astronomy) ,KINEMATICS ,IMAGE processing ,VARIABLE stars - Abstract
We present new high-contrast images in near-infrared wavelengths (λ
c = 1.04, 1.24, 1.62, 2.18, and 3.78 μm) of the young variable star CQ Tau, aiming to constrain the presence of companions in the protoplanetary disc. We reached a Ks -band contrast of 14 mag with SPHERE/IRDIS at separations greater than 0 |${_{.}^{\prime\prime}}$| 4 from the star. Our mass sensitivity curve rules out giant planets above 4 MJup immediately outside the spiral arms at ∼60 au and above 2–3 MJup beyond 100 au to 5σ confidence assuming hot-start models. We do, however, detect four spiral arms, a double-arc and evidence for shadows in scattered light cast by a misaligned inner disc. Our observations may be explained by an unseen close-in companion on an inclined and eccentric orbit. Such a hypothesis would also account for the disc CO cavity and disturbed kinematics. [ABSTRACT FROM AUTHOR]- Published
- 2022
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