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dc.contributor.author | Thomas, RD | en_US |
dc.contributor.author | Togi, A | en_US |
dc.contributor.author | Verstraete, L | en_US |
dc.contributor.author | Witt, AN | en_US |
dc.contributor.author | Wootten, A | en_US |
dc.contributor.author | Ysard, N | en_US |
dc.contributor.author | Zettergren, H | en_US |
dc.contributor.author | Zhang, Y | en_US |
dc.contributor.author | Zhang, ZE | en_US |
dc.contributor.author | Zhen, J | en_US |
dc.date.accessioned | 2024-03-07T08:13:35Z | |
dc.date.issued | 2024-03 | en_US |
dc.identifier.uri | https://qmro.qmul.ac.uk/xmlui/handle/123456789/95121 | |
dc.description.abstract | 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. | en_US |
dc.format.extent | 988 - 992 | en_US |
dc.language | eng | en_US |
dc.relation.ispartof | Science | en_US |
dc.title | A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk. | en_US |
dc.type | Article | |
dc.rights.holder | © 2024 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. | |
dc.identifier.doi | 10.1126/science.adh2861 | en_US |
pubs.author-url | https://www.ncbi.nlm.nih.gov/pubmed/38422128 | en_US |
pubs.issue | 6686 | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 383 | en_US |
rioxxterms.funder | Default funder | en_US |
rioxxterms.identifier.project | Default project | en_US |
qmul.funder | Dorothy Hodgkin Fellowship::Royal Society | en_US |