The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Differential Rotation and Turbulence in Extended H i Disks
Open accessAbstract
When present, extended disks of neutral hydrogen around spiral galaxies show a remarkably uniform velocity dispersion of ~6 km s -1 . Since stellar winds and supernovae are largely absent in such regions, neither the magnitude nor the constancy of this number can be accounted for in the classical picture in which interstellar turbulence is driven by stellar energy sources. Here we suggest that magnetic fields with strengths of a few microgauss in these extended disks allow energy to be extracted from galactic differential rotation through MHD-driven turbulence. The magnitude and constancy of the observed velocity dispersion may be understood if its value is Alfvénic. Moreover, by providing a simple explanation for a lower bound to the gaseous velocity fluctuations, MHD processes may account for the sharp outer edge to star formation in galaxy disks.
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Citations
Cites
Synthetic properties of starburst galaxies
Leitherer, C., & Heckman, T. M. (1995) · The Astrophysical Journal Supplement Series · doi:10.1086/192112 · Cited by 672 · cited 1×
“A high estimate for the SNR for this SFR is 10−12 SN pc−2 yr−1 (e.g. Leitherer & Heckman 1995).”
BackgroundThe galactic fountain of high-velocity clouds
Bregman, J. N. (1980) · The Astrophysical Journal · doi:10.1086/157776 · Cited by 610 · cited 1×
“Infall models include the returns from a galactic fountain (Bregman 1980; Schulman et al. 1996), or chimney (Norman & Ikeuchi 1989), or simply the direct accretion of external intergalactic matter (Tóth & Ostriker 1992; Kamphuis & Sancisi 1993).”
Background
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
Star Formation Thresholds and Galaxy Edges: Why and Where
Schaye, J. (2004) · The Astrophysical Journal · doi:10.1086/421232 · Cited by 615
Star Formation Thresholds in Galactic Disks
Martin, C. L., & Kennicutt, Jr. (2001) · The Astrophysical Journal · doi:10.1086/321452 · Cited by 490
Accretion-driven turbulence as universal process: galaxies, molecular clouds, and protostellar disks
Klessen, R. S., & Hennebelle, P. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913780 · Cited by 301
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
- Sellwood, J. A., & Balbus, S. A.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1999-02
- Volume
- 511
- Issue
- 2
- Pages
- 660-665
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2069271107
- Cited by
- 219
- References
- 2
- FWCI
- 8.00
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Sellwood, J. A., & Balbus, S. A. (1999). Differential Rotation and Turbulence in Extended H i Disks. The Astrophysical Journal. https://doi.org/10.1086/306728
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