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Verfasst von:Chevance, Mélanie [VerfasserIn]   i
 Kruijssen, Diederik [VerfasserIn]   i
 Hygate, Alexander P. S. [VerfasserIn]   i
 Schruba, Andreas [VerfasserIn]   i
 Longmore, Steven N [VerfasserIn]   i
 Groves, Brent [VerfasserIn]   i
 Henshaw, Jonathan D. [VerfasserIn]   i
 Herrera, Cinthya N [VerfasserIn]   i
 Hughes, Annie [VerfasserIn]   i
 Jeffreson, Sarah [VerfasserIn]   i
 Lang, Philipp [VerfasserIn]   i
 Leroy, Adam K [VerfasserIn]   i
 Meidt, Sharon E. [VerfasserIn]   i
 Pety, Jérôme [VerfasserIn]   i
 Razza, Alessandro [VerfasserIn]   i
 Rosolowsky, Erik [VerfasserIn]   i
 Schinnerer, Eva [VerfasserIn]   i
 Bigiel, Frank [VerfasserIn]   i
 Blanc, Guillermo A [VerfasserIn]   i
 Emsellem, Eric [VerfasserIn]   i
 Faesi, Christopher M [VerfasserIn]   i
 Glover, Simon [VerfasserIn]   i
 Haydon, Daniel T. [VerfasserIn]   i
 Ho, I-Ting [VerfasserIn]   i
 Kreckel, Kathryn [VerfasserIn]   i
 Lee, Janice C [VerfasserIn]   i
 Liu, Daizhong [VerfasserIn]   i
 Querejeta, Miguel [VerfasserIn]   i
 Saito, Toshiki [VerfasserIn]   i
 Sun, Jiayi [VerfasserIn]   i
 Usero, Antonio [VerfasserIn]   i
 Utomo, Dyas [VerfasserIn]   i
Titel:The lifecycle of molecular clouds in nearby star-forming disc galaxies
Verf.angabe:Mélanie Chevance, JM Diederik Kruijssen, Alexander PS Hygate, Andreas Schruba, Steven N Longmore, Brent Groves, Jonathan D Henshaw, Cinthya N Herrera, Annie Hughes, Sarah MR Jeffreson, Philipp Lang, Adam K Leroy, Sharon E Meidt, Jérôme Pety, Alessandro Razza, Erik Rosolowsky, Eva Schinnerer, Frank Bigiel, Guillermo A Blanc, Eric Emsellem, Christopher M Faesi, Simon CO Glover, Daniel T Haydon, I-Ting Ho, Kathryn Kreckel, Janice C Lee, Daizhong Liu, Miguel Querejeta, Toshiki Saito, Jiayi Sun, Antonio Usero and Dyas Utomo
Jahr:2020
Umfang:38 S.
Fussnoten:Advance access publication 2019 December 19 ; Gesehen am 15.04.2021
Titel Quelle:Enthalten in: Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society
Ort Quelle:Oxford : Oxford Univ. Press, 1827
Jahr Quelle:2020
Band/Heft Quelle:493(2020), 2 vom: Apr., Seite 2872-2909
ISSN Quelle:1365-2966
Abstract:It remains a major challenge to derive a theory of cloud-scale (≲100 pc) star formation and feedback, describing how galaxies convert gas into stars as a function of the galactic environment. Progress has been hampered by a lack of robust empirical constraints on the giant molecular cloud (GMC) lifecycle. We address this problem by systematically applying a new statistical method for measuring the evolutionary timeline of the GMC lifecycle, star formation, and feedback to a sample of nine nearby disc galaxies, observed as part of the PHANGS-ALMA survey. We measure the spatially resolved (∼100 pc) CO-to-H α flux ratio and find a universal de-correlation between molecular gas and young stars on GMC scales, allowing us to quantify the underlying evolutionary timeline. GMC lifetimes are short, typically $10\!-\!30\,{\rm Myr}$, and exhibit environmental variation, between and within galaxies. At kpc-scale molecular gas surface densities ΣH2≥8M⊙pc−2, the GMC lifetime correlates with time-scales for galactic dynamical processes, whereas at ΣH2≤8M⊙pc−2 GMCs decouple from galactic dynamics and live for an internal dynamical time-scale. After a long inert phase without massive star formation traced by H α (75-90 per cent of the cloud lifetime), GMCs disperse within just 1-5 Myr once massive stars emerge. The dispersal is most likely due to early stellar feedback, causing GMCs to achieve integrated star formation efficiencies of 4-10 per cent. These results show that galactic star formation is governed by cloud-scale, environmentally dependent, dynamical processes driving rapid evolutionary cycling. GMCs and H ii regions are the fundamental units undergoing these lifecycles, with mean separations of 100−300 pc in star-forming discs. Future work should characterize the multiscale physics and mass flows driving these lifecycles.
DOI:doi:10.1093/mnras/stz3525
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext: https://doi.org/10.1093/mnras/stz3525
 DOI: https://doi.org/10.1093/mnras/stz3525
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1754996086
Verknüpfungen:→ Zeitschrift

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