9 papers · 1 filter
A correlation between accretion and outflow rates for Class II Young Stellar Objects with full and transition disks
A. A. Rota, N. van der Marel, A. Garufi +7
Magnetothermal (MHD) winds and jets originate in a wide range of regions of protoplanetary disks (1-30 au) and are thought to be the primary mechanisms driving accretion onto the c…
Protoplanetary disk insights from the first ERIS/APP survey at 4 μm
F. Maio, V. Roccatagliata, D. Fedele +17
We present high-contrast imaging observations of seven protoplanetary disks at 4um using the ERIS on the VLT. This study focuses on detecting scattered light from micron-sized dust…
The centimeter emission from planet-forming disks in Taurus
Antonio Garufi, Carlos Carrasco-Gonzalez, Enrique Macias +16
The last decade has witnessed remarkable advances in the characterization of the (sub-)millimeter emission from planet-forming disks. Instead, the study of the (sub-)centimeter emi…
The two-dimensional pressure structure of the HD 163296 protoplanetary disk as probed by multi-molecule kinematics
V. Pezzotta, S. Facchini, C. Longarini +2
[Abridged] Gas kinematics is a new and unique way to study planet-forming environments by an accurate characterization of disk velocity fields. High angular resolution ALMA observa…
Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Dynamical Evidence of a Spiral-Arm-Driving and Gap-Opening Protoplanet from SAO 206462 Spiral Motion
Chen Xie, Chengyan Xie, Bin B. Ren +8
In the early stages of planetary system formation, young exoplanets gravitationally interact with their surrounding environments and leave observable signatures on protoplanetary d…
Resolved ALMA observations of water in the inner astronomical units of the HL Tau disk
Stefano Facchini, Leonardo Testi, Elizabeth Humphreys +7
The water molecule is a key ingredient in the formation of planetary systems, with the water snowline being a favourable location for the growth of massive planetary cores. Here we…