Journal: Astronomy and Astrophysics

  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): II. The radial structure of debris discs
    Context. Debris discs are populated by belts of planetesimals, whose structure carries dynamical imprints of planets and the formation and evolutionary history...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): III. The vertical structure of debris disks
    Context. Debris disks ─ collisionally sustained belts of dust and sometimes gas around main sequence stars ─ are remnants of planet formation processes and are...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): IV. CO gas imaging and overview
    Context. CO gas is detected in a significant number (~20) of debris discs (exoKuiper belts), but understanding its origin and evolution remains elusive. Crucial...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): IX. Gas-driven origin for the continuum arc in the debris disc of HD121617
    Context. Debris discs were long considered to be largely gas-free environments, where dynamical evolution is governed primarily by collisional fragmentation...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): V. Comparison between scattered light and thermal emission
    Context. Debris discs are analogues to our own Kuiper belt around main-sequence stars and are therefore referred to as exoKuiper belts. They have been resolved...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): VI. Asymmetries and offsets
    Context. Asymmetries in debris discs provide unique clues to understand the evolution and architecture of planetary systems. Previous studies of debris discs at...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): VII. Optically thick gas with broad CO gaussian local line profiles in the HD 121617 disc
    Context. CO gas has been detected in ~20 debris discs, typically classified as CO-poor or CO-rich. We present observations of the CO-rich HD 121617 debris disc...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): VIII. A dust arc and non-Keplerian gas kinematics in HD 121617
    Context. ExoKuiper belts around young A-type stars often host CO gas, whose origin is still unclear. The ALMA survey to Resolve exoKuiper belt Substructures...
  • Publication
    The ALMA survey to Resolve exoKuiper belt Substructures (ARKS): X. Interpreting the peculiar dust rings around HD 131835
    Context. Dusty discs detected around main-sequence stars are thought to be signs of planetesimal belts in which the dust distribution is shaped by collisional...