The Kelvin–Helmholtz instability in the Orion nebula: the effect of radiation pressure-Reference-Cited by-同舟云学术

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The Kelvin–Helmholtz instability in the Orion nebula: the effect of radiation pressure

Published:2017-05-29 Issue:3 Volume:470 Page:2559-2565
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Yaghouti S. Akram¹,Nejad-Asghar Mohsen²,Abbassi Shahram¹³

Affiliation:

1. Department of Physics, School of Science, Ferdowsi University of Mashhad, Mashhad 91775-1436, Iran

2. Department of Physics, University of Mazandaran, Babolsar 47416-13534, Iran

3. School of Astronomy, Institute for Studies in Theoretical Physics and Mathematics, Tehran 19395-5531, Iran

Funder

Ferdowsi University of Mashhad

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/470/3/2559/18245536/stx1327.pdf

Reference22 articles.

1. Physical Conditions in Orion’s Veil

2. THE KELVIN-HELMHOLTZ INSTABILITY IN ORION: A SOURCE OF TURBULENCE AND CHEMICAL MIXING

3. Waves on the surface of the Orion molecular cloud

4. Magnetic Fields in Molecular Clouds

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1. Effect of Transverse Magnetic Field on Kelvin–Helmholtz Instability in the Presence of a Radiation Field;The Astrophysical Journal;2024-07-01

2. Evidence of Kelvin-Helmholtz and tearing mode instabilities at the magnetopause during space weather events;Frontiers in Astronomy and Space Sciences;2024-05-09

3. Kelvin–Helmholtz instability in sheared dusty plasma flows including dust polarization and ion drag forces;Physica Scripta;2022-05-17

4. Effects of head loss, surface tension, viscosity and density ratio on the Kelvin–Helmholtz instability in different types of pipelines;Physica D: Nonlinear Phenomena;2021-10

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