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A statistical view on the galactic cold ISM distribution

Published online by Cambridge University Press:  05 March 2015

L. Viktor Tóth ,
Sarolta Zahorecz ,
Gábor Marton  and
Erika Verebélyi
L. Viktor Tóth
Affiliation:
Department of Astronomy, Eötvös University, Budapest email: l.v.toth@astro.elte.hu
Sarolta Zahorecz
Affiliation:
Department of Astronomy, Eötvös University, Budapest email: l.v.toth@astro.elte.hu
Gábor Marton
Affiliation:
Department of Astronomy, Eötvös University, Budapest email: l.v.toth@astro.elte.hu
Erika Verebélyi
Affiliation:
Department of Astronomy, Eötvös University, Budapest email: l.v.toth@astro.elte.hu
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Abstract

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Inhomogenities 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.

Keywords

ISM: dustISM: moleculesISM: bubblesISM: cloudsstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 579
Copyright
Copyright © International Astronomical Union 2015 

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