The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)
California Institute of Technology · Astronomical Observatory · +32 more institutions
Abstract
Context . Debris discs are populated by belts of planetesimals, whose structure carries dynamical imprints of planets and the formation and evolutionary history of the planetary system. The relatively faint emission of debris discs has previously made it challenging to obtain a large sample of high-resolution ALMA images to characterise their substructures. Aims . The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) was recently completed to cover the lack of high-resolution observations and to investigate the prevalence of substructures such as radial gaps and rings in a sample of 24 debris discs. This study characterises the radial structure of debris discs in the ARKS programme. Methods . We…
Citation impact
- FWCI
- 108.09
- Percentile
- 100%
- References
- 137
Authors
41Topics & keywords
- Planetesimal
- Debris
- Planet
- Debris disk
- Population
- Planetary system
- Halo
- Deconvolution
Funding
- NSNational Science and Technology CouncilAward: NSTC 112-2112-M-001-032-MY3
- NSNational Science FoundationAwards: DGE 2140743, AST-2307920
- NANational Aeronautics and Space AdministrationAwards: HST-AR-16608.001-A, 80NSSC23K0288
- URUK Research and Innovation
- HFHeising-Simons Foundation
- RSRoyal SocietyAward: URF-R1-221669
- ANAgence Nationale de la RechercheAward: ANR-21-CE31-0015
- IRIrish Research CouncilAwards: GOIPG/2022/1895, IRCLA- 2022-3788
- NKNemzeti Kutatási Fejlesztési és Innovációs HivatalAwards: TKP2021-NKTA-64, ADVANCED 149943
- ANAgencia Nacional de Investigación y DesarrolloAward: NCN2024_001
- H2Horizon 2020 Framework ProgrammeAward: 101004719
- EREuropean Research CouncilAward: 100117693
- EREuropean Regional Development FundAward: PID2023-153342NB-I00/10.13039/501100011033
- AEAgencia Estatal de Investigación
- HEHORIZON EUROPE European Research CouncilAward: 101064124