activity
20242026
collaborators

6 papers

astro-ph.EP2026

Destructuring the disk of AB Aurigae: Dynamics and accretion

Anthony Boccaletti, Emmanuel Di Folco, Anne Dutrey +23

In this paper, we present near-IR polarized images of the AB Aur disk at three epochs spanning 3.85 years with SPHERE/IRDIS, as well as Halpha images obtained with SPHERE/ZIMPOL at…

astro-ph.EP2026

Young system development in a cometary globule: An investigation into the eccentric disk around AT Pyx in terms of planet-formation and interaction with its surrounding environment

Dan McLachlan, Christian Ginski, Jake Byrne +5

This paper presents new data and analyses of the AT Pyx system, a disk-hosting young star located in a cometary globule in the Gum Nebula. This radiation-driven structure is an unu…

astro-ph.EP2025

Imaging the LkCa 15 system in polarimetry and total intensity without self-subtraction artefacts

C. Swastik, Zahed Wahhaj, Myriam Benisty +7

Studying young protoplanetary disks is essential for understanding planet formation, but traditional angular differential imaging can introduce self-subtraction artefacts that hind…

astro-ph.IM2025

Debris disks and their properties with the Habitable Worlds Observatory

Isabel Rebollido, Yasuhiro Hasegawa, Meredith MacGregor +5

The study of the last stages of planet formation, also known as debris disks, is fundamental to place constrains on the formation of planetary sized bodies. Debris disks are compos…

astro-ph.IM2025

Studying Protoplanets and Protoplanetary Disks with the Habitable Worlds Observatory

Bin B. Ren

Since the discovery of the first exoplanet orbiting a Sun-like star, the confirmation of nearly 6000 exoplanets to date - and their diversity - has revolutionized our knowledge of…

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…