Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients-Reference-Cited by-同舟云学术

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Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients

Published:2011-10 Issue:7368 Volume:478 Page:214-217
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Gaensler B. M.,Haverkorn M.,Burkhart B.,Newton–McGee K. J.,Ekers R. D.,Lazarian A.,McClure–Griffiths N. M.,Robishaw T.,Dickey J. M.,Green A. J.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature10446.pdf

Reference30 articles.

1. Ferrière, K. M. The interstellar environment of our galaxy. Rev. Mod. Phys. 73, 1031–1066 (2001)

2. de Avillez, M. A. & Breitschwerdt, D. Global dynamical evolution of the ISM in star forming galaxies. I. High resolution 3D simulations: effect of the magnetic field. Astron. Astrophys. 436, 585–600 (2005)

3. Chepurnov, A. & Lazarian, A. Extending the big power law in the sky with turbulence spectra from Wisconsin Hα Mapper data. Astrophys. J. 710, 853–858 (2010)

4. Armstrong, J. W., Rickett, B. J. & Spangler, S. R. Electron density power spectrum in the local interstellar medium. Astrophys. J. 443, 209–221 (1995)

5. Kritsuk, A. G., Norman, M. L., Padoan, P. & Wagner, R. The statistics of supersonic isothermal turbulence. Astrophys. J. 665, 416–431 (2007)

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