The DOI matches its Crossref record; 79 of the 79 references it cites were found in a registry or an index.
On the onset of galactic winds in quiescent star forming galaxies
Open accessAbstract
Context.The hierarchical model of galaxy formation, despite its many successes, still overpredicts the baryons fraction locked in galaxies as a condensed phase. The efficiency of supernovae feedback, proposed a long time ago as a possible solution for this so-called “overcooling” problem, is still under debate, mainly because modelling supernovae explosions within a turbulent interstellar medium, while capturing realistic large scale flows around the galaxy is a very demanding task.
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Citations
Cites
The Luminosity Function and Stellar Evolution.
Salpeter, E. E. (1955) · The Astrophysical Journal · doi:10.1086/145971 · Cited by 8,697
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 8×
“In this paper, we report the first self–consistent adaptive mesh refinement (AMR) simulation of a collapsing NFW (Navarro et al. 1996) spherical cloud forming a galactic disk from the inside out.”
MethodInfluentialThe Global Schmidt Law in Star‐forming Galaxies
Kennicutt, Jr. (1998) · The Astrophysical Journal · doi:10.1086/305588 · Cited by 5,202
On the Gravitational Stability of a Disk of Stars
Toomre, A. (1964) · The Astrophysical Journal · doi:10.1086/147861 · Cited by 3,349 · cited 1×
“In this way, we can reproduce a stiffer equation of state for the dense gas, leading to thicker, more stable discs (Toomre 1964, Robertson et al. 2004).”
MethodCooling functions for low-density astrophysical plasmas
Sutherland, R. S., & Dopita, M. A. (1993) · The Astrophysical Journal Supplement Series · doi:10.1086/191823 · Cited by 2,434
Galaxy formation through hierarchical clustering
White, S. D. M., & Frenk, C. S. (1991) · The Astrophysical Journal · doi:10.1086/170483 · Cited by 2,354
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
Cosmological hydrodynamics with adaptive mesh refinement: A new high resolution code called RAMSES
Teyssier, R. (2002) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20011817 · Cited by 2,187
Self-citationMcKee, C. F., & Ostriker, J. P. (1977) · The Astrophysical Journal · doi:10.1086/155667 · Cited by 2,082 · cited 2×
“This value, comparable to the typical size of galactic superbubbles (McKee & Ostriker 1977), is however larger than individual supernovae remmants, whose size just before the snow plow phase varies from 10 to 50 pc, depending on the exact early shock wave dynamics, whether adiabatic or…”
BackgroundCole, S., Lacey, C. G., Baugh, C. M., & Frenk, C. S. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2000.03879.x · Cited by 1,952
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
Cosmic rays in a galactic breeze
Taylor, A. M., & Giacinti, G. (2017) · Physical Review D · doi:10.1103/physrevd.95.023001 · Cited by 18
Metadata
- Authors
- Dubois, Y., & Teyssier, R.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2007-10-23
- Volume
- 477
- Issue
- 1
- Pages
- 79-94
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W1970587228
- Cited by
- 296
- References
- 79
- FWCI
- 6.04
- Type
- journal article
- Language
- en
- Open access
- bronze
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.