Inefficient jet-induced star formation in Centaurus A

Q. Salomé; P. Salomé; M.-A. Miville-Deschênes; F. Combes; S. Hamer

doi:10.1051/0004-6361/201731429e

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Volume 617 (September 2018)

A&A, 617 (2018) C3

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201731429]

Issue		A&A Volume 617, September 2018


Article Number		C3
Number of page(s)		1
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/201731429e
Published online		25 September 2018

A&A 617, C3 (2018)

High resolution ALMA observations of the northern filaments^⋆ (Corrigendum)

Q. Salomé¹, P. Salomé², M.-A. Miville-Deschênes¹, F. Combes²^,3 and S. Hamer⁴

¹ Institut d’Astrophysique Spatiale, CNRS, Université Paris-Sud, Université Paris-Saclay, bâtiment 121, 91405 Orsay cedex, France
e-mail: quentin.salome@ias.u-psud.fr
² LERMA, Observatoire de Paris, PSL Research Univ., CNRS, Sorbonne Université, UPMC Université Paris 06, 75014 Paris, France
³ Collège de France, 11 place Marcelin Berthelot, 75005 Paris, France
⁴ CRAL, Observatoire de Lyon, CNRS, Université Lyon 1, 9 Avenue Ch. André, 69561 Saint Genis Laval cedex, France

Key words: methods:data analysis / galaxies:individual:Centaurus A / galaxies:star formation / galaxies:interactions / galaxies:evolution / radio lines:galaxies / errata, addenda

^⋆

A catalogue of the molecular clouds is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/608/A98

Erratum for: A&A 608, A98 (2017), https://doi.org/10.1051/0004-6361/201731429

The table published in Appendix A was an old version and differs from our catalogue of molecular clouds. We provide a new version of Table A.1, which shows the correct values of the radius and the molecular gas mass for the first molecular clouds. A catalogue of all the GMCs is available at the CDS.

Table A.1.

Properties of some molecular clouds extracted with the method presented in Sect. 2.2.

© ESO 2018

All Tables

Table A.1.

Properties of some molecular clouds extracted with the method presented in Sect. 2.2.

In the text

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