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Characteristic scale of star formation - I. Clump formation efficiency on local scales

Eden, DJ, Moore, TJT, Plume, R, Rigby, AJ, Urquhart, JS, Marsh, KA, Penaloza, CH, Clark, PC, Smith, MWL, Tahani, K, Ragan, SE, Thompson, MA, Johnstone, D, Parsons, H and Rani, R (2020) Characteristic scale of star formation - I. Clump formation efficiency on local scales. Monthly Notices of the Royal Astronomical Society, 500 (1). pp. 191-210. ISSN 0035-8711

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Abstract

We have used the ratio of column densities derived independently from the 850-μm continuum James Clerk Maxwell Telescope Plane Survey and the 13CO/C18O (J = 3 → 2) Heterodyne Inner Milky Way Plane Survey to produce maps of the dense-gas mass fraction (DGMF) in two slices of the Galactic plane centred at ℓ = 30° and 40°. The observed DGMF is a metric for the instantaneous clump formation efficiency (CFE) in the molecular gas. We split the two fields into velocity components corresponding to the spiral arms that cross them, and a two-dimensional power-spectrum analysis of the spiral-arm DGMF maps reveals a break in slope at the approximate size scale of molecular clouds. We interpret this as the characteristic scale of the amplitude of variations in the CFE and a constraint on the dominant mechanism regulating the CFE and, hence, the star formation efficiency in CO-traced clouds.

Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2020 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Uncontrolled Keywords: 0201 Astronomical and Space Sciences
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press
Related URLs:
Date Deposited: 22 Nov 2021 11:26
Last Modified: 22 Nov 2021 11:26
DOI or ID number: 10.1093/mnras/staa3188
URI: https://researchonline.ljmu.ac.uk/id/eprint/15812
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