The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
Disc-halo interaction -- I. Three-dimensional evolution of the Galactic disc
Open accessAbstract
The results of a three-dimensional model for disc-halo interaction are presented here. The model considers explicitly the input of energy and mass by isolated and correlated supernovae in the disc. Once disrupted by the explosions, the disc never returns to its initial state. Instead it approaches a state where a thin H i disc is formed in the Galactic plane, overlaid by thick H i and H ii gas discs with scaleheights of 500 pc and 1–1.5 kpc, respectively. The upper parts of the thick H ii disc (the diffuse ionized medium) act as a disc-halo interface, and its formation and stability are directly correlated to the supernova rate per unit area in the simulated disc.
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Cites
McKee, C. F., & Ostriker, J. P. (1977) · The Astrophysical Journal · doi:10.1086/155667 · Cited by 2,082 · cited 1×
“Furthermore, chimneys reduce the volume filling factor of the hot gas in the disk reducing it from 0.7 predicted by the three-phase model of McKee & Ostriker (1977) to some 0.2 as predicted by Norman & Ikeuchi (1989).”
MethodInfluentialConsequences of a New Hot Component of the Interstellar Medium
Shapiro, P. R., & Field, G. B. (1976) · The Astrophysical Journal · doi:10.1086/154332 · Cited by 714 · cited 1×
“These comprise two major models: the classical fountain (CF) model (Shapiro & Field, 1976; Bregman, 1980; Kahn, 1981) and the chimney model (Tomisaka & Ikeuchi, 1986; Norman & Ikeuchi, 1989).”
BackgroundThe galactic fountain of high-velocity clouds
Bregman, J. N. (1980) · The Astrophysical Journal · doi:10.1086/157776 · Cited by 610 · cited 1×
“These comprise two major models: the classical fountain (CF) model (Shapiro & Field, 1976; Bregman, 1980; Kahn, 1981) and the chimney model (Tomisaka & Ikeuchi, 1986; Norman & Ikeuchi, 1989).”
BackgroundThe H I halo in the inner galaxy
Lockman, F. J. (1984) · The Astrophysical Journal · doi:10.1086/162277 · Cited by 200 · cited 14×
“Isolated and clustered supernovae of types Ib, Ic and II occur in the volume V at rates obtained from the values discussed in §2.1 and given by σ V VG = 1.42 × 10−3σ yr−1 (7) where VG = 1.4×1011 pc3 is the volume of the Galactic disk with a radius of 15 kpc and a thickness of 200 pc, and σ is the rate of supernovae ob…”
BackgroundInfluential
Cited by
Control of star formation by supersonic turbulence
Mac Low, M.-M., & Klessen, R. S. (2004) · Reviews of Modern Physics · doi:10.1103/revmodphys.76.125 · Cited by 1,761
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
Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
Hartmann, L., Ballesteros‐Paredes, J., & Bergin, E. A. (2001) · The Astrophysical Journal · doi:10.1086/323863 · Cited by 567
Strickland, D. K., Heckman, T. M., Colbert, E. J. M., Hoopes, C. G., & Weaver, K. A. (2004) · The Astrophysical Journal Supplement Series · doi:10.1086/382214 · Cited by 368
Turbulent Structure of a Stratified Supernova‐driven Interstellar Medium
Joung, M. K. R., & Mac Low, M. (2006) · The Astrophysical Journal · doi:10.1086/508795 · Cited by 296
Metadata
- Authors
- de Avillez, M. A.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2000-07-01
- Volume
- 315
- Issue
- 3
- Pages
- 479-497
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2129445184
- Cited by
- 188
- References
- 4
- FWCI
- 7.41
- Type
- journal article
- Language
- en
- Open access
- green
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- de Avillez, M. A. (2000). Disc-halo interaction -- I. Three-dimensional evolution of the Galactic disc. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2000.03464.x
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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.
