The Origin of the H I Holes in the Interstellar Medium of Holmberg II

Details The Origin of the H I Holes in the Interstellar Medium of Holmberg II The Origin of the H I Holes in the Interstellar Medium of Holmberg II

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.292..135d&link_type=abstract

Astrophysics and Space Science, v. 292, Issue 1, p. 135-140 (2004).

Astronomy and Astrophysics

Astrophysics

6

Dwarf Galaxies, Holmberg Ii, Ism, Turbulence

Scientific paper

We use a comparison between the autocorrelation length value in 21-cm hi maps of Holmberg II and the autocorrelation length derived from simulated maps in order to constrain the physical processes that are responsible for the observed distribution of holes and shells in the interstellar medium (ISM) of the galaxy. Our results show that large scale turbulence coupled to a weak cooling can reproduce the value of the autocorrelation length which is observed.

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