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| Verfasst von: | Orr, Matthew [VerfasserIn]  |
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| | Hatchfield, H. Perry [VerfasserIn] |
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| | Battersby, Cara [VerfasserIn] |
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| | Hayward, Christopher C. [VerfasserIn] |
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| | Hopkins, Philip F. [VerfasserIn] |
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| | Wetzel, Andrew [VerfasserIn] |
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| | Benincasa, Samantha M. [VerfasserIn] |
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| | Loebman, Sarah R. [VerfasserIn] |
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| | Sormani, Mattia C. [VerfasserIn] |
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| | Klessen, Ralf S. [VerfasserIn] |
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| Titel: | Fiery cores |
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| Titelzusatz: | bursty and smooth star formation distributions across galaxy centers in cosmological zoom-in simulations |
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| Verf.angabe: | Matthew E. Orr, H. Perry Hatchfield, Cara Battersby, Christopher C. Hayward, Philip F. Hopkins, Andrew Wetzel, Samantha M. Benincasa, Sarah R. Loebman, Mattia C. Sormani, and Ralf S. Klessen |
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| E-Jahr: | 2021 |
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| Jahr: | 2021 February 19 |
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| Umfang: | 7 S. |
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| Fussnoten: | Gesehen am 08.04.2021 |
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| Titel Quelle: | Enthalten in: The astrophysical journal / 2 |
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| Ort Quelle: | London : Institute of Physics Publ., 1995 |
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| Jahr Quelle: | 2021 |
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| Band/Heft Quelle: | 908(2021), 2, Artikel-ID L31, Seite 1-7 |
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| ISSN Quelle: | 2041-8213 |
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| Abstract: | We present an analysis of the R ≲ 1.5 kpc core regions of seven simulated Milky Way-mass galaxies, from the FIRE-2 (Feedback in Realistic Environments) cosmological zoom-in simulation suite, for a finely sampled period (Δt = 2.2 Myr) of 22 Myr at z ≈ 0, and compare them with star formation rate (SFR) and gas surface density observations of the Milky Way’s Central Molecular Zone (CMZ). Despite not being tuned to reproduce the detailed structure of the CMZ, we find that four of these galaxies are consistent with CMZ observations at some point during this 22 Myr period. The galaxies presented here are not homogeneous in their central structures, roughly dividing into two morphological classes; (a) several of the galaxies have very asymmetric gas and SFR distributions, with intense (compact) starbursts occurring over a period of roughly 10 Myr, and structures on highly eccentric orbits through the CMZ, whereas (b) others have smoother gas and SFR distributions, with only slowly varying SFRs over the period analyzed. In class (a) centers, the orbital motion of gas and star-forming complexes across small apertures (R ≲ 150 pc, analogously ∣l∣ < 1° in the CMZ observations) contributes as much to tracers of star formation/dense gas appearing in those apertures, as the internal evolution of those structures does. These asymmetric/bursty galactic centers can simultaneously match CMZ gas and SFR observations, demonstrating that time-varying star formation can explain the CMZ’s low star formation efficiency. |
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| DOI: | doi:10.3847/2041-8213/abdebd |
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| 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/10.3847/2041-8213/abdebd |
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| | DOI: https://doi.org/10.3847/2041-8213/abdebd |
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| Datenträger: | Online-Ressource |
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| Sprache: | eng |
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| K10plus-PPN: | 1753332168 |
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| Verknüpfungen: | → Zeitschrift |
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