First results from SMAUG: insights into star formation conditions from spatially resolved ISM properties in TNG50

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Bibliographische Detailangaben
Hauptverfasser: Motwani, Bhawna (VerfasserIn) , Genel, Shy (VerfasserIn) , Bryan, Greg L. (VerfasserIn) , Kim, Chang-Goo (VerfasserIn) , Pandya, Viraj (VerfasserIn) , Somerville, Rachel S. (VerfasserIn) , Smith, Matthew C. (VerfasserIn) , Ostriker, Eve C. (VerfasserIn) , Nelson, Dylan (VerfasserIn) , Pillepich, Annalisa (VerfasserIn) , Forbes, John C. (VerfasserIn) , Belfiore, Francesco (VerfasserIn) , Pakmor, Rüdiger (VerfasserIn) , Hernquist, Lars (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2022 February 18
In: The astrophysical journal
Year: 2022, Jahrgang: 926, Heft: 2, Pages: 1-24
ISSN:1538-4357
DOI:10.3847/1538-4357/ac3d2d
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.3847/1538-4357/ac3d2d
Volltext
Verfasserangaben:Bhawna Motwani, Shy Genel, Greg L. Bryan, Chang-Goo Kim, Viraj Pandya, Rachel S. Somerville, Matthew C. Smith, Eve C. Ostriker, Dylan Nelson, Annalisa Pillepich, John C. Forbes, Francesco Belfiore, Rüdiger Pakmor, and Lars Hernquist

MARC

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