Molecular clouds have power-law probability distribution functions (not log-normal)

Author(s)
Joao Alves, Marco Lombardi, Charles Lada
Abstract

We investigate the shape of the probability distribution of column

densities (PDF) in molecular clouds. Through the use of low-noise,

extinction-calibrated Planck-Herschel emission data for eight molecular

clouds, we demonstrate that, contrary to common belief, the PDFs of

molecular clouds are not described well by log-normal functions, but are

instead power laws with exponents close to two and with breaks between

AK≃0.1 and 0.2mag, so close to the CO self-shielding limit and not

far from the transition between molecular and atomic gas. Additionally,

we argue that the intrinsic functional form of the PDF cannot be

securely determined below AK≃0.1mag, limiting our ability to

investigate more complex models for the shape of the cloud PDF.

Organisation(s)
Department of Astrophysics
External organisation(s)
Università degli Studi di Milano-Bicocca, Harvard-Smithsonian Center for Astrophysics
Journal
IAU General Assembly Meeting
Volume
29
Publication date
08-2015
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Portal url
https://ucrisportal.univie.ac.at/en/publications/2119c487-41b5-4667-9baa-952111e8bc13