Molecular clouds have power-law probability distribution functions

Autor(en)
Marco Lombardi, João Alves, Charles J. Lada
Abstrakt

In this Letter we investigate the shape of the probability distribution of column densities (PDF) in molecular clouds. Through the use of low-noise, extinction-calibrated Herschel/Planck 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 A

K ≃ 0.1 and 0.2 mag, 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 A

K ≃ 0.1 mag, limiting our ability to investigate more complex models for the shape of the cloud PDF.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Harvard-Smithsonian Center for Astrophysics, Università degli Studi di Milano-Bicocca
Journal
Astronomy & Astrophysics
Band
576
Anzahl der Seiten
4
ISSN
0004-6361
DOI
https://doi.org/10.1051/0004-6361/201525650
Publikationsdatum
03-2015
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Schlagwörter
ASJC Scopus Sachgebiete
Astronomy and Astrophysics, Space and Planetary Science
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/molecular-clouds-have-powerlaw-probability-distribution-functions(1de34621-9387-4e93-b38d-c96b368b38ef).html