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...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| 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
|
| Verfasserangaben: | J.D. Henshaw, S.N. Longmore and J.M.D. Kruijssen |
| Zusammenfassung: | © 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... |
|---|---|
| Beschreibung: | Gesehen am 24.10.2017 |
| Beschreibung: | Online Resource |
| ISSN: | 1745-3933 |
| DOI: | 10.1093/mnrasl/slw237 |