The DOI matches its Crossref record; 79 of the 79 references it cites were found in a registry or an index.
An analytic model for the evolution of the stellar, gas and metal content of galaxies: An analytic model for galaxy evolution
Open accessAbstract
We present an analytic formalism that describes the evolution of the stellar, gas and metal content of galaxies. It is based on the idea, inspired by hydrodynamic simulations, that galaxies live in a slowly evolving equilibrium between inflow, outflow and star formation. We argue that this formalism broadly captures the behaviour of galaxy properties evolving in simulations. The resulting equilibrium equations for the star formation rate, gas fraction and metallicity depend on three key free parameters that represent ejective feedback, preventive feedback and reaccretion of ejected material. We schematically describe how these parameters are constrained by models and observations. Galaxies perturbed off the equilibrium relations owing to inflow stochasticity tend to be driven back towards equilibrium, such that deviations in star formation rate at a given mass are correlated with gas fraction and anticorrelated with metallicity. After an early gas accumulation epoch, quiescently star-forming galaxies are expected to be in equilibrium over most of cosmic time. The equilibrium model provides a simple intuitive framework for understanding the cosmic evolution of galaxy properties, and centrally features the cycle of baryons between galaxies and surrounding gas as the driver of galaxy growth.
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Cites
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Cited by
The EAGLE project: simulating the evolution and assembly of galaxies and their environments
Schaye, J., Crain, R. A., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., Dalla Vecchia, C., Frenk, C. S., McCarthy, I. G., Helly, J. C., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2058 · Cited by 3,601
The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
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Lilly, S. J., Carollo, C. M., Pipino, A., Renzini, A., & Peng, Y. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/772/2/119 · Cited by 870
CONSTRAINING THE LOW-MASS SLOPE OF THE STAR FORMATION SEQUENCE AT 0.5 <z< 2.5
Whitaker, K. E., Franx, M., Leja, J., van Dokkum, P. G., Henry, A., Skelton, R. E., Fumagalli, M., Momcheva, I. G., Brammer, G. B., Labbé, I., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/795/2/104 · Cited by 854
Dusty star-forming galaxies at high redshift
Casey, C. M., Narayanan, D., & Cooray, A. (2014) · Physics Reports · doi:10.1016/j.physrep.2014.02.009 · Cited by 800
Metadata
- Authors
- Davé, R., Finlator, K., & Oppenheimer, B. D.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2011-12
- Pages
- no-no
- ISSN
- 0035-8711 (ISSN-L)
- OpenAlex
- W2141444467
- Cited by
- 512
- References
- 79
- FWCI
- 15.38
- Type
- journal article
- Language
- en
- Open access
- green
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- Davé, R., Finlator, K., & Oppenheimer, B. D. (2011). An analytic model for the evolution of the stellar, gas and metal content of galaxies: An analytic model for galaxy evolution. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2011.20148.x
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