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Cited by 202

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Galaxy morphology and star formation in the Illustris Simulation at z = 0

Open access
Snyder, Gregory F., Torrey, Paul, Lotz, Jennifer M., Genel, Shy, McBride, Cameron K., Vogelsberger, Mark, Pillepich, Annalisa, Nelson, Dylan, Sales, Laura V., Sijacki, Debora, Hernquist, Lars, Springel, Volker·2015·Monthly Notices of the Royal Astronomical Society

Abstract

We study how optical galaxy morphology depends on mass and star formation rate (SFR) in the Illustris Simulation. To do so, we measure automated galaxy structures in 10 808 simulated galaxies at z = 0 with stellar masses 109.7 < M*/Mȯ < 1012.3. We add observational realism to idealized synthetic images and measure non-parametric statistics in rest-frame optical and near-IR images from four directions. We find that Illustris creates a morphologically diverse galaxy population, occupying the observed bulge strength locus and reproducing median morphology trends versus stellar mass, SFR, and compactness. Morphology correlates realistically with rotation, following classification schemes put forth by kinematic surveys. Type fractions as a function of environment agree roughly with data. These results imply that connections among mass, star formation, and galaxy structure arise naturally from models matching global star formation and halo occupation functions when simulated with accurate methods. This raises a question of how to construct experiments on galaxy surveys to better distinguish between models. We predict that at fixed halo mass near 1012 Mȯ, disc-dominated galaxies have higher stellar mass than bulge-dominated ones, a possible consequence of the Illustris feedback model. While Illustris galaxies at M* ∼ 1011 Mȯ have a reasonable size distribution, those at M* ∼ 1010 Mȯ have half-light radii larger than observed by a factor of 2. Furthermore, at M* ∼ 1010.5–1011 Mȯ, a relevant fraction of Illustris galaxies have distinct ‘ring-like’ features, such that the bright pixels have an unusually wide spatial extent.

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Metadata

Authors
Snyder, G. F., Torrey, P., Lotz, J. M., Genel, S., McBride, C. K., Vogelsberger, M., Pillepich, A., Nelson, D., Sales, L. V., Sijacki, D., Hernquist, L., & Springel, V.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2015-10-08
Volume
454
Issue
2
Pages
1886-1908
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W1801137374
Cited by
202
References
4
FWCI
13.50
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Galaxy morphology and star formation in the Illustris Simulation at z = 0. https://app.cochat.ai/papers/10.1093/mnras/stv2078
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Snyder, G. F., Torrey, P., Lotz, J. M., Genel, S., McBride, C. K., Vogelsberger, M., Pillepich, A., Nelson, D., Sales, L. V., Sijacki, D., Hernquist, L., & Springel, V. (2015). Galaxy morphology and star formation in the Illustris Simulation at z = 0. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stv2078

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