Some of the observed large-scale motions, especially those associated with warps of the gas layer, may be driven by gas infall.
Interstellar Turbulence I: Observations and Processes
Oxford University Press is a department of the University of Oxford. It furthers the University's objective of excellence in research, scholarship, and education by publishing worldwide. Sign In or Create an Account.
Sign In. Advanced Search. Article Navigation.
- Sprinkle with Murder.
- Support Independent Student Journalism?
- Depolarization canals and interstellar turbulence.
- Community Palliative Care: The Role of the Clinical Nurse Specialist.
Close mobile search navigation Article Navigation. Volume Article Contents. Stellar kinematics and interstellar turbulence Richard B.
- Interstellar Turbulence!
- Donate to arXiv?
- Turbulence in the Local Interstellar Medium and the IBEX Ribbon [SSA] | arXiver.
- Legal Counsel: Book 2: Frequently Asked Questions About the Law.
- Reggio Emilia 2007 2008!
- American Electricians Handbook?
- Thermal Instability-induced Interstellar Turbulence!
Oxford Academic. Google Scholar. Cite Citation.
- Near-Earth Objects: Finding Them Before They Find Us;
- Numerical simulations of compressively driven interstellar turbulence.
- BDPI USP - Detalhe do registro: Turbulence in the interstellar medium.
- Algebraic Geometry 3: Further Study of Schemes (Translations of Mathematical Monographs Vol. 218).
- Pump users handbook;
Permissions Icon Permissions. Abstract Data assembled from a variety of sources show that the velocity dispersion of young stars and cool interstellar gas increases systematically with the size of the region considered, over a wide range of length scales. Department of Astronomy Sterling Hall N.
Feedback, questions or accessibility issues:. University of Wisconsin-Madison Department of Astronomy.
endorisand.cf Kowal, A. For our tests we make use of three-dimensional compressible MHD isothermal simulations performed for different sonic, i. We introduce the bispectrum, a new tool for statistical studies of the interstellar medium which, unlike an ordinary power spectrum of turbulence, preserves the phase information of the stochastic field. We show that the bispectra of the three-dimensional stochastic density field and of column densities, available from observations, are similar.