Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-13T06:49:40.722Z Has data issue: false hasContentIssue false
  • English
  • Français

Intense velocity-shears, magnetic fields and filaments in diffuse gas

Published online by Cambridge University Press:  05 March 2015

Edith Falgarone ,
Pierre Hily-Blant ,
François Levrier ,
Manuel Berthet ,
Pierre Bastien  and
Dan Clemens
Edith Falgarone
Affiliation:
LERMA/LRA, Ecole Normale Supérieure & Observatoire de Paris, 24 rue Lhomond, 75005 Paris, France email: edith.falgarone@ens.fr
Pierre Hily-Blant
Affiliation:
IPAG, Observatoire de Grenoble, St Martin d'Hères, France
François Levrier
Affiliation:
LERMA/LRA, Ecole Normale Supérieure & Observatoire de Paris, 24 rue Lhomond, 75005 Paris, France email: edith.falgarone@ens.fr
Manuel Berthet
Affiliation:
LERMA/LRA, Ecole Normale Supérieure & Observatoire de Paris, 24 rue Lhomond, 75005 Paris, France email: edith.falgarone@ens.fr
Pierre Bastien
Affiliation:
University of Montréal, Montréal, Canada
Dan Clemens
Affiliation:
Institute for Astrophysical Research, Boston University, Boston, USA
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The dissipation of turbulence is a key process in the evolution of diffuse gas towards denser structures. The vast range of coupled scales and the variety of dissipative processes in interstellar turbulence make it a complex system to analyze. Observations now provide powerful statistics of the gas velocity field, density and magnetic field orientations, opening a rich field of investigation. On-going comparisons of the orientation of intense velocity-shears, magnetic field and tenuous filaments of matter in a turbulent high-latitude cloud are promising.

Keywords

TurbulenceMagnetic FieldsISM: moleculesISM: kinematics and dynamicsISM: generalISM: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 388
Copyright
Copyright © International Astronomical Union 2015 

References

Clemens, D. P., Pinnick, A. F. & Pavel, M. D., 2012 ApJS, 200, 20CrossRefGoogle Scholar
Falgarone, E., Pety, J., & Hily-Blant, P., 2009, A&A, 507, 355Google Scholar
Hily-Blant, P., Falgarone, E. & Pety, J., 2008 A&A 481, 367Google Scholar