A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk
成果类型:
Article
署名作者:
Berne, Olivier; Habart, Emilie; Peeters, Els; Schroetter, Ilane; Canin, Amelie; Sidhu, Ameek; Chown, Ryan; Bron, Emeric; Haworth, Thomas J.; Klaassen, Pamela; Trahin, Boris; Van De Putte, Dries; Alarcon, Felipe; Zannese, Marion; Abergel, Alain; Bergin, Edwin A.; Bernard-Salas, Jeronimo; Boersma, Christiaan; Cami, Jan; Cuadrado, Sara; Dartois, Emmanue; Dicken, Daniel; Elyajouri, Meriem; Fuente, Asuncion; Goicoeche, Javier R.; Gordon, Karl D.; Issa, Lina; Joblin, Christine; Kannavou, Olga; Khan, Baria; Lacinbala, Ozan; Languignon, David; Le Gai, Romane; Maragkoudakis, Alexandros; Meshaka, Raphael; Okada, Yoko; Onaka, Takashi; Pasquini, Sofia; Pound, Marc W.; Robberto, Massimo; Rollig, Markus; Schefter, Bethany; Schirmer, Thiebaut; Simmer, Thomas; Tabone, Benoit; Tielens, Alexander G. G. M.; Vicente, Silvia; Wolfire, Mark G.
署名单位:
Centre National de la Recherche Scientifique (CNRS); Universite de Toulouse; Universite Toulouse III - Paul Sabatier; Centre National de la Recherche Scientifique (CNRS); Universite Paris Saclay; Sorbonne Universite; Western University (University of Western Ontario); Western University (University of Western Ontario); Universite PSL; Observatoire de Paris; Sorbonne Universite; University of London; University College London; Queen Mary University London; Space Telescope Science Institute; University of Michigan System; University of Michigan; National Aeronautics & Space Administration (NASA); NASA Ames Research Center; Consejo Superior de Investigaciones Cientificas (CSIC); CSIC - Instituto de Fisica Fundamental (IFF); Centre National de la Recherche Scientifique (CNRS); Universite Paris Saclay; Consejo Superior de Investigaciones Cientificas (CSIC); CSIC - Centro de Astrobiologia (INTA); Johns Hopkins University; Centre National de la Recherche Scientifique (CNRS); Institut de Planetologie et d'Astrophysique de Grenoble (IPAG); Communaute Universite Grenoble Alpes; Universite Grenoble Alpes (UGA); University of Cologne; University of Tokyo; Meisei University; University System of Maryland; University of Maryland College Park; Chalmers University of Technology; Leiden University; Leiden University - Excl LUMC
刊物名称:
SCIENCE
ISSN/ISSBN:
0036-9208
DOI:
10.1126/science.adh2861
发表日期:
2024-03-01
页码:
988-992
关键词:
external photoevaporation
orion-nebula
circumstellar disks
massive stars
radiation
dust
destruction
dispersal
emission
clusters
摘要:
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.