Erratum to: Seeding the galactic centre gas stream: gravitational instabilities set the initial conditions for the formation of protocluster clouds

© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Societyerrata, addenda, stars: formation, ISM: clouds, ISM: kinematics and dynamics, ISM: structure, Galaxy: centre, Galaxy: kinematics and dynamics...The paper ‘Seeding the Galactic Centre gas stream: gravit...

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Hauptverfasser: Henshaw, Jonathan D. (VerfasserIn) , Longmore, Steven N. (VerfasserIn) , Kruijssen, Diederik (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 08 October 2016
In: Monthly notices of the Royal Astronomical Society. Letters
Year: 2017, Jahrgang: 466, Heft: 1, Pages: L13-L13
ISSN:1745-3933
DOI:10.1093/mnrasl/slw237
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnrasl/slw237
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Verfasserangaben:J.D. Henshaw, S.N. Longmore and J.M.D. Kruijssen

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520 |a © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Societyerrata, addenda, stars: formation, ISM: clouds, ISM: kinematics and dynamics, ISM: structure, Galaxy: centre, Galaxy: kinematics and dynamics...The paper ‘Seeding the Galactic Centre gas stream: gravitational instabilities set the initial conditions for the formation of protocluster clouds’ was originally published in MNRAS, 463, L122 (2016).After online publication of Henshaw, Longmore & Kruijssen (2016), we discovered a number of errors in Table 1. Due to an integer division error, the number densities presented are a factor of 4/3 greater than they should be. Additionally, the tabulated densities refer to atomic hydrogen number densities (μ = 1.4), not molecular hydrogen number densities (μ = 2.8, as claimed). These two errors propagated into the computation of the free-fall times. To summarize, the number densities and free-fall... 
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