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Verfasst von:Jackson, Thomas M. [VerfasserIn]   i
 Pasquali, Anna [VerfasserIn]   i
 Pacifici, Camilla [VerfasserIn]   i
 Engler, Christoph [VerfasserIn]   i
 Pillepich, Annalisa [VerfasserIn]   i
 Grebel, Eva K. [VerfasserIn]   i
Titel:The stellar mass assembly of low-redshift, massive, central galaxies in SDSS and the TNG300 simulation
Verf.angabe:Thomas M. Jackson, A. Pasquali, C. Pacifici, C. Engler, A. Pillepich and E.K. Grebel
E-Jahr:2020
Jahr:07 August 2020
Umfang:14 S.
Fussnoten:Gesehen am 22.12.2020
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:497(2020), 4, Seite 4262-4275
ISSN Quelle:1365-2966
Abstract:The stellar mass assembly of galaxies can be affected by both secular and environmental processes. In this study, for the first time, we investigate the stellar mass assembly of similar to 90 000 low-redshift, central galaxies selected from SDSS group catalogues (M-Stellar greater than or similar to 109.5 M-circle dot, M-Halo greater than or similar to 10(12) M-circle dot) as a function of both stellar mass and halo mass. We use estimates of the times at which 10, 50, and 90 per cent of the stellar mass were assembled from photometric spectral energy distribution fitting, allowing a more complete investigation than single stellar ages alone. We consider trends in both stellar mass and halo mass simultaneously, finding dependences of all assembly times on both. We find that galaxies with higher stellar masses (at constant halo mass) have on average older lookback times, similar to previous studies of galaxy assembly. We also find that galaxies at higher halo mass (at constant stellar mass) have younger lookback times, possibly due to a larger reservoir of gas for star formation. An exception to this is a subsample with high stellar-to-halo mass ratios, which are likely massive, field spirals. We compare these observed trends to those predicted by the TNG300 simulation, finding good agreement overall as a function of either stellar mass or halo mass. However, some differences in the assembly times (of up to similar to 3 Gyr) appear when considering both stellar mass and halo mass simultaneously, noticeably at intermediate stellar masses (M-Stellar similar to 10(11) M-circle dot). These discrepancies are possibly linked to the quenched fraction of galaxies and the kinetic mode active galactic nucleus feedback implemented in TNG300.
DOI:doi:10.1093/mnras/staa2306
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/staa2306
 DOI: https://doi.org/10.1093/mnras/staa2306
Datenträger:Online-Ressource
Sprache:eng
Sach-SW:catalog
 dark
 data release
 galaxies: evolution
 galaxies: formation
 galaxies: groups: general
 illustristng simulations
 matter
 physical-properties
 population synthesis
 simple-model
 size evolution
 star-formation rates
K10plus-PPN:1743482965
Verknüpfungen:→ Zeitschrift

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