Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, H16(10), p. 579-579, 2012
DOI: 10.1017/s1743921314012253
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A statistical view on the galactic cold ISM distribution
Journal article published in 2012 by
L. Viktor Tóth,
Sarolta Zahorecz,
Gábor Marton 
,
Erika Verebélyi
,
Erika Verebélyi
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
AbstractInhomogenities were found in the distribution of the cold fraction in the interstellar medium (traced by Planck cold clumps). In large scales there is a significant overdensity on some shells, in small scales there are elongated groups. Critical column density for star formation is N(H2) = 7 × 1021 cm−2.
