Large-scale galactic turbulence: can self-gravity drive the observed H i velocity dispersions?
- 1 January 2009
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 392 (1) , 294-308
- https://doi.org/10.1111/j.1365-2966.2008.14043.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 62 references indexed in Scilit:
- The turbulent interstellar mediumComptes Rendus Physique, 2006
- The Supernova Rate–Velocity Dispersion Relation in the Interstellar MediumThe Astrophysical Journal, 2006
- Global dynamical evolution of the ISM in star forming galaxiesAstronomy & Astrophysics, 2005
- Volume filling factors of the ISM phases in star forming galaxiesAstronomy & Astrophysics, 2004
- Simulations of normal spiral galaxiesMonthly Notices of the Royal Astronomical Society, 2003
- Dark matter and visible baryons in M33Monthly Notices of the Royal Astronomical Society, 2003
- An H I absorption survey of M31 and M33 - The mixture of warm and cool phases in the interstellar media of spiral galaxiesThe Astrophysical Journal, 1993
- A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolutionThe Astrophysical Journal, 1991
- NGC 1058 - Gas motions in an extended, quiescent spiral diskThe Astrophysical Journal, 1990
- Multi-level adaptive solutions to boundary-value problemsMathematics of Computation, 1977