A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk
Artikel i vetenskaplig tidskrift, 2024
Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiation produces photodissociation regions (PDRs) on the surfaces of protoplanetary disks around low-mass stars, which affects planet formation within the disks. We report James Webb Space Telescope and Atacama Large Millimeter Array observations of a FUV-irradiated protoplanetary disk in the Orion Nebula. Emission lines are detected from the PDR; modeling their kinematics and excitation allowed us to constrain the physical conditions within the gas. We quantified the mass-loss rate induced by the FUV irradiation and found that it is sufficient to remove gas from the disk in less than a million years. This is rapid enough to affect giant planet formation in the disk.
Författare
O. Berné
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Emilie Habart
Institut d'Astrophysique Spatiale
Els Peeters
Western University
Ilane Schroetter
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Amelie Canin
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Ameek Sidhu
Western University
Ryan Chown
Western University
E. Bron
Centre national de la recherche scientifique (CNRS)
Thomas J. Haworth
Queen Mary University of London
Pamela Klaassen
Royal Observatory
Boris Trahin
Institut d'Astrophysique Spatiale
Dries Van De Putte
Space Telescope Science Institute (STScI)
Felipe Alarcon
University of Michigan
Marion Zannese
Institut d'Astrophysique Spatiale
Alain Abergel
Institut d'Astrophysique Spatiale
E. A. Bergin
University of Michigan
J. Bernard-Salas
Centre d’Etudes et de Recherche de Grasse
Christiaan Boersma
National Aeronautics and Space Administration (NASA)
Jan Cami
Western University
S. Cuadrado
Consejo Superior de Investigaciones Científicas (CSIC)
E. Dartois
Université Paris-Saclay
D. Dicken
Institut d'Astrophysique Spatiale
Meriem Elyajouri
Institut d'Astrophysique Spatiale
A. Fuente
Instituto Nacional de Tecnica Aeroespacial
J.R. Goicoechea
Consejo Superior de Investigaciones Científicas (CSIC)
K. Gordon
Space Telescope Science Institute (STScI)
Lina Issa
Institut de Recherche en Astrophysique et Planétologie (IRAP)
C. Joblin
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Olga Kannavou
Institut d'Astrophysique Spatiale
Baria Khan
Western University
Ozan Lacinbala
Institut d'Astrophysique Spatiale
David Languignon
Centre national de la recherche scientifique (CNRS)
R. Le Gal
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Alexandros Maragkoudakis
National Aeronautics and Space Administration (NASA)
Raphael Meshaka
Institut d'Astrophysique Spatiale
Yoko Okada
Universität zu Köln
Takashi Onaka
University of Tokyo
Sofia Pasquini
Western University
Marc W. Pound
University of Maryland
Massimo Robberto
Space Telescope Science Institute (STScI)
M. Rollig
Universität zu Köln
Bethany Schefter
Western University
Thiébaut-Antoine Schirmer
Institut d'Astrophysique Spatiale
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Thomas Simmer
Institut d'Astrophysique Spatiale
Benoît Tabone
Institut d'Astrophysique Spatiale
A.G.G.M. Tielens
University of Maryland
S. Vicente
Instituto de Astrofísica e Ciências do Espaço (IA)
M.G. Wolfire
University of Maryland
Science
20965672 (ISSN) 25773585 (eISSN)
Vol. 383 6686 988-992Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.1126/science.adh2861
PubMed
38422128