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# Inefficient jet-induced star formation in Centaurus A. High resolution ALMA observations of the northern filaments (Corrigendum)

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

► To cite this version:

Q. Salomé, P. Salomé, M. -A. Miville-Deschênes, F. Combes, S. Hamer. Inefficient jet-induced star formation in Centaurus A. High resolution ALMA observations of the northern filaments (Corrigendum). Astronomy & Astrophysics - A&A, 2018, 617, 10.1051/0004-6361/201731429e. insu-03711219

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https://insu.hal.science/insu-03711219v1

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# Inefficient jet-induced star formation in Centaurus A

## High resolution ALMA observations of the northern filaments* (Corrigendum)

Q. Salomé<fnref n="1" />, P. Salomé<fnref n="2" />, M.-A. Miville-Deschênes<fnref n="1" />, F. Combes<fnref n="2" />,<fnref n="3" />, and S. Hamer<fnref n="4" />

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

**Key words.** methods:sdata analysis – galaxies:individual:Centaurus A – galaxies:star formation – galaxies:interactions – galaxies:evolution – radio lines:galaxies – errata, addenda

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><caption>**Table A.1.** Properties of some molecular clouds extracted with the method presented in Sect. 2.2.</caption><thead><tr><th>Clump</th><th>R<br>(pc)</th><th>S<sub>CO</sub>Δν<br>(Jy km s<sup>-1</sup>)</th><th>ν<sub>cent</sub><br>(km s<sup>-1</sup>)</th><th>Δν<br>(km s<sup>-1</sup>)</th><th>M<sub>H<sub>2</sub></sub><br>(M<sub>☉</sub>)</th><th>Σ<sub>H<sub>2</sub></sub><br>(M<sub>☉</sub> pc<sup>-2</sup>)</th></tr></thead><tbody><tr><td>1</td><td>27.24</td><td>2.909</td><td>-180.97</td><td>16.65</td><td>4.41 × 10<sup>5</sup></td><td>98.86</td></tr><tr><td>2</td><td>27.56</td><td>2.338</td><td>-275.31</td><td>11.01</td><td>3.54 × 10<sup>5</sup></td><td>103.14</td></tr><tr><td>3</td><td>21.78</td><td>1.591</td><td>-228.34</td><td>11.58</td><td>2.41 × 10<sup>5</sup></td><td>100.06</td></tr><tr><td>4</td><td>28.01</td><td>3.579</td><td>-227.82</td><td>20.20</td><td>5.43 × 10<sup>5</sup></td><td>125.01</td></tr><tr><td>5</td><td>22.68</td><td>1.841</td><td>-186.42</td><td>14.60</td><td>2.79 × 10<sup>5</sup></td><td>96.46</td></tr><tr><td>6</td><td>25.76</td><td>1.907</td><td>-226.01</td><td>14.67</td><td>2.89 × 10<sup>5</sup></td><td>77.97</td></tr><tr><td>7</td><td>35.82</td><td>3.359</td><td>-202.54</td><td>12.97</td><td>5.09 × 10<sup>5</sup></td><td>86.64</td></tr><tr><td>8</td><td>29.68</td><td>1.271</td><td>-206.29</td><td>5.73</td><td>1.93 × 10<sup>5</sup></td><td>49.17</td></tr><tr><td>9</td><td>21.37</td><td>1.101</td><td>-176.68</td><td>10.77</td><td>1.67 × 10<sup>5</sup></td><td>68.35</td></tr><tr><td>10</td><td>19.03</td><td>0.774</td><td>-223.42</td><td>14.97</td><td>1.17 × 10<sup>5</sup></td><td>76.30</td></tr></tbody></table>

**Notes.** The velocities are relative to Cen A ($v_{LSR} \sim 545$ km s$^{-1}$). Note that the table contains the FWHM, while the online catalogue provides the velocity dispersion $\sigma_v$ (there is a factor of 2.354 between the two).

<footnote n="1">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</footnote>

<footnote n="2">² LERMA, Observatoire de Paris, PSL Research Univ., CNRS, Sorbonne Université, UPMC Université Paris 06, 75014 Paris, France</footnote>

<footnote n="3">³ Collège de France, 11 place Marcelin Berthelot, 75005 Paris, France</footnote>

<footnote n="4">⁴ CRAL, Observatoire de Lyon, CNRS, Université Lyon 1, 9 Avenue Ch. André, 69561 Saint Genis Laval cedex, France</footnote>

<footnote>* 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</footnote>