Is the Parker Instability a Viable Mechanism for the Formation of Giant Molecular Clouds?

Details Is the Parker Instability a Viable Mechanism for the Formation of Giant Molecular Clouds? Is the Parker Instability a Viable Mechanism for the Formation of Giant Molecular Clouds?

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.292..255k&link_type=abstract

Astrophysics and Space Science, v. 292, Issue 1, p. 255-260 (2004).

Astronomy and Astrophysics

Astrophysics

3

Instabilities, Cosmic Rays, Ism:Magnetic Fields, Mhd

Scientific paper

The stratified interstellar medium has been known to be subject to the Parker instability, and the instability has been considered as a plausible mechanism for the formation of giant molecular clouds (GMCs). By presenting our recent efforts to understand the instability through linear analyses and numerical simulations, we raise a negative point of view that the Parker instability alone could not form GMCs.

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