activity
20242026
collaborators

6 papers

astro-ph.SR2026

A Quiet Host in an Active Planet-Forming Disk: Optical Spectroscopy of WISPIT 2

C. Swastik, M. Bestha, L. S. Sonith +11

WISPIT 2 is a young pre-main-sequence star hosting a multi-ringed transition disk and two directly imaged protoplanets, including the accreting WISPIT 2b, making it the closest kno…

astro-ph.EP2025

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…

astro-ph.EP2025

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…

astro-ph.EP2025

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…

astro-ph.EP2025

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…

astro-ph.EP2024

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…