UV-driven chemistry as a signpost of late-stage planet formation
UV-driven chemistry as a signpost of late-stage planet formation
About this item
Full title
Author / Creator
Calahan, Jenny K. , Bergin, Edwin A. , Bosman, Arthur D. , Rich, Evan A. , Andrews, Sean M. , Bergner, Jennifer B. , Cleeves, L. Ilsedore , Guzmán, Viviana V. , Huang, Jane , Ilee, John D. , Law, Charles J. , Le Gal, Romane , Öberg, Karin I. , Teague, Richard , Walsh, Catherine , Wilner, David J. and Zhang, Ke
Publisher
London: Nature Publishing Group UK
Journal title
Language
English
Formats
Publication information
Publisher
London: Nature Publishing Group UK
Subjects
More information
Scope and Contents
Contents
The chemical reservoir within protoplanetary disks has a direct impact on planetary compositions and the potential for life. A long-lived carbon- and nitrogen-rich chemistry at cold temperatures (≤ 50 K) is observed within cold and evolved planet-forming disks. This is evidenced by bright emission from small organic radicals in 1–10 Myr aged system...
Alternative Titles
Full title
UV-driven chemistry as a signpost of late-stage planet formation
Authors, Artists and Contributors
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2768590234
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2768590234
Other Identifiers
ISSN
2397-3366
E-ISSN
2397-3366
DOI
10.1038/s41550-022-01831-8
