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Verfasst von:Winter, Andrew J. [VerfasserIn]   i
 Haworth, Thomas [VerfasserIn]   i
Titel:The external photoevaporation of planet-forming discs
Verf.angabe:Andrew J. Winter, Thomas J. Haworth
E-Jahr:2022
Jahr:14 October 2022
Umfang:41 S.
Fussnoten:Gesehen am 29.11.2022
Titel Quelle:Enthalten in: The European physical journal / Plus
Ort Quelle:Berlin : Springer, 2011
Jahr Quelle:2022
Band/Heft Quelle:137(2022), 10, Artikel-ID 1132, Seite 1-41
ISSN Quelle:2190-5444
Abstract:Planet-forming disc evolution is not independent of the star formation and feedback process in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses discs in a process called ‘external photoevaporation’. This process is understood to be the dominant environmental influence acting on planet-forming discs in typical star-forming regions. Our best studied discs are nearby, in sparse stellar groups where external photoevaporation is less effective. However, the majority of discs are expected to reside in much stronger UV environments. Understanding external photoevaporation is therefore key to understanding how most discs evolve, and hence, how most planets form. Here, we review our theoretical and observational understanding of external photoevaporation. We also lay out key developments for the future to address existing unknowns and establish the full role of external photoevaporation in the disc evolution and planet formation process.
DOI:doi:10.1140/epjp/s13360-022-03314-1
URL:kostenfrei: Volltext: https://doi.org/10.1140/epjp/s13360-022-03314-1
 DOI: https://doi.org/10.1140/epjp/s13360-022-03314-1
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1823827462
Verknüpfungen:→ Zeitschrift
 
 
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