activity
20232025
most citedCharacterization of debris disks observed with SPHERE

8 citations · 15 across the 7 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2025★ 8 cited

Characterization of debris disks observed with SPHERE

N. Engler, J. Milli, N. Pawellek +33

This study aims to characterize debris disks observed with SPHERE across multiple programs, with the goal of identifying systematic trends in disk morphology, dust mass, and grain…

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…

astro-ph.EP2024★ 4 cited

Multi-band reflectance and shadowing of RX J1604.3-2130 protoplanetary disk in scattered light

Huisheng Zhong, Bin B. Ren, Bo Ma +5

Context.Spatially-resoved cicrumstellar disk spectrum and composition can provide valuable insights into the bulk composition of forming planets, as well as the mineralogical signa…

astro-ph.EP2023

A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion

Bin B. Ren, Chen Xie, Myriam Benisty +8

While there have been nearly two dozen of spiral arms detected from planet-forming disks in near-infrared scattered light, none of their substellar drivers have been confirmed. By…

astro-ph.EP2023★ 3 cited

The first scattered light images of HD 112810, a faint debris disk in the Sco-Cen association

Elisabeth C. Matthews, Mickaël Bonnefoy, Chen Xie +17

Context: Circumstellar debris disks provide insight into the formation and early evolution of planetary systems. Resolved belts in particular help to locate planetesimals in exosys…

astro-ph.CO2023

Are "Changing-Look'' Active Galactic Nuclei Special in the Coevolution of Supermassive Black Holes and their Hosts? I

J. Wang, W. K. Zheng, T. G. Brink +5

The nature of the so-called ``changing-look'' (CL) active galactic nucleus (AGN), which is characterized by spectral-type transitions within ~yr, remains an open question.…