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A statistical view on the galactic cold ISM distribution
Published online by Cambridge University Press: 05 March 2015
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.
- 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
References
Wright, E. L., Eisenhardt, P. R. M., Mainzer, A. K., et al. 2010, AJ 140, 1868CrossRefGoogle Scholar
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