Bipolar Outflow and Turbulence in Molecular Clouds Due to Protostellar Alfvén Waves

Symposium - International Astronomical Union
doi 10.1017/s0074180900090513
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

Protostellar Turbulence in Cluster Forming Regions of Molecular Clouds

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Chemical Effects of Shear Alfvén Waves in Molecular Clouds

Symposium - International Astronomical Union
1992English

Nature of Turbulence, Dissipation, and Heating in Space Plasmas: From Alfvén Waves to Kinetic Alfvén Waves

Journal of Geophysical Research: Space Physics
2016English

Turbulence and Magnetic Fields in Molecular Clouds

Symposium - International Astronomical Union
1991English

From Clouds to Protostellar Cores

Symposium - International Astronomical Union
2004English

Conditions for Sustainment of Magnetohydrodynamic Turbulence Driven by Alfvén Waves

Physics of Plasmas
Condensed Matter Physics
2001English

MagnetoHydrodynamic Shock Waves in Molecular Clouds

Symposium - International Astronomical Union
1991English

MagnetoHydrodynamic Shock Waves in Molecular Clouds

Symposium - International Astronomical Union
1991English

Comparison of Turbulence in HII Regions and Molecular Clouds

Symposium - International Astronomical Union
1991English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy