The DOI matches its Crossref record; 56 of the 56 references it cites were found in a registry or an index.
Star formation and feedback in smoothed particle hydrodynamic simulations – I. Isolated galaxies
Open accessAbstract
We present an analysis of star formation and feedback recipes appropriate for galactic smoothed particle hydrodynamics simulations. Using an isolated Milky Way-like galaxy, we constrain these recipes based on well-established observational results. Our star formation recipe is based on that of Katz with the additional inclusion of physically motivated supernova feedback recipes. We propose a new feedback recipe in which Type II supernovae are modelled using an analytical treatment of blastwaves. With this feedback mechanism and a tuning of other star formation parameters, the star formation in our isolated Milky Way-like galaxy follows the slope and normalization of the observed Schmidt law. In addition, we reproduce the low-density cut-off and filamentary structure of star formation observed in disc galaxies. Our final recipe will enable better comparison of N-body simulations with observations.
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Cites
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
The Global Schmidt Law in Star‐forming Galaxies
Kennicutt, Jr. (1998) · The Astrophysical Journal · doi:10.1086/305588 · Cited by 5,202
Smoothed Particle Hydrodynamics
Monaghan, J. J. (1992) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.30.090192.002551 · Cited by 4,957
Dickey, J. M., & Lockman, F. J. (1990) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.28.090190.001243 · Cited by 4,492
The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
Woosley, S. E., & Weaver, T. A. (1995) · The Astrophysical Journal Supplement Series · doi:10.1086/192237 · Cited by 3,761
Embedded Clusters in Molecular Clouds
Lada, C. J., & Lada, E. A. (2003) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.41.011802.094844 · Cited by 3,034
Schmidt, M. (1959) · The Astrophysical Journal · doi:10.1086/146614 · Cited by 2,420
Springel, V., & Hernquist, L. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06206.x · Cited by 2,262
McKee, C. F., & Ostriker, J. P. (1977) · The Astrophysical Journal · doi:10.1086/155667 · Cited by 2,082 · cited 10×
“Therefore, we implemented an effective version of supernova feedback that uses the blastwave solution presented in McKee & Ostriker (1977).”
BackgroundMethodResultInfluentialFilippenko, A. V. (1997) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.35.1.309 · Cited by 1,824
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
Dark matter self-interactions and small scale structure
Tulin, S., & Yu, H.-B. (2018) · Physics Reports · doi:10.1016/j.physrep.2017.11.004 · Cited by 1,111
Theoretical Challenges in Galaxy Formation
Naab, T., & Ostriker, J. P. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-040019 · Cited by 722
The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
Grand, R. J. J., Gómez, F. A., Marinacci, F., Pakmor, R., Springel, V., Campbell, D. J. R., Frenk, C. S., Jenkins, A., & White, S. D. M. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx071 · Cited by 557
Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks
Roškar, R., Debattista, V. P., Quinn, T. R., Stinson, G. S., & Wadsley, J. (2008) · The Astrophysical Journal · doi:10.1086/592231 · Cited by 501
Self-citation
Metadata
- Authors
- Stinson, G., Seth, A., Katz, N., Wadsley, J., Governato, F., & Quinn, T.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2006-11-13
- Volume
- 373
- Issue
- 3
- Pages
- 1074-1090
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2126399417
- Cited by
- 746
- References
- 56
- FWCI
- 8.87
- Type
- journal article
- Language
- en
- Open access
- bronze
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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