# Erratum: Kinematics of the Atomic ISM in M33 on 80 pc scales

Eric Koch, Erik Rosolowsky, Felix Lockman, Amanda Kepley, Adam Leroy, Andreas Schruba, J. Braine, Julianne Dalcanton, Megan Johnson, Snežana Stanimirović

► To cite this version:

Eric Koch, Erik Rosolowsky, Felix Lockman, Amanda Kepley, Adam Leroy, et al.. Erratum: Kinematics of the Atomic ISM in M33 on 80 pc scales. Monthly Notices of the Royal Astronomical Society, 2018, 480 (3), pp.3193-3194. 10.1093/mnras/sty2137. hal-01868057

HAL Id: hal-01868057

https://hal.science/hal-01868057v1

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# Erratum: Kinematics of the Atomic ISM in M33 on 80 pc scales

by Eric W. Koch,<sup>1★</sup> Erik W. Rosolowsky,<sup>1★</sup> Felix J. Lockman,<sup>2</sup> Amanda A. Kepley,<sup>3</sup> Adam Leroy,<sup>4</sup> Andreas Schruba,<sup>5</sup> Jonathan Braine,<sup>6</sup> Julianne Dalcanton,<sup>7</sup> Megan C. Johnson<sup>8</sup> and Snežana Stanimirović<sup>9</sup>

**Key words:** ISM: kinematics and dynamics – radio lines: ISM – galaxies: ISM – galaxies: individual: M33 – erratum.

The paper 'Kinematics of the Atomic ISM ifigun M33 on 80 pc scales' was published in Mon. Not. R. Astron. Soc. **479**, 2505–2533 (2018). During the editorial process, a typo was introduced into the title of the paper. The correct title is 'Kinematics of the Atomic ISM in M33 on 80 pc scales.'

Table C1 also contained incorrect radial bin values for the reported units. We present the corrected values here in Table 1. This error only occurred in the table and has no effect on the results.

<footnote n="1"><sup>1</sup>University of Alberta, Department of Physics, 4-183 CCIS, Edmonton AB T6G 2E1, Canada</footnote>

<footnote n="2"><sup>2</sup>Green Bank Observatory, PO Box 2, Green Bank, WV 24944, USA</footnote>

<footnote n="3"><sup>3</sup>National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA</footnote>

<footnote n="4"><sup>4</sup>The Ohio State University, Department of Astronomy, 140 West 18th Avenue, Columbus, OH 43210, USA</footnote>

<footnote n="5"><sup>5</sup>Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße 1, D-85748 Garching, Germany</footnote>

<footnote n="6"><sup>6</sup>Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France</footnote>

<footnote n="7"><sup>7</sup>Department of Astronomy, Box 351580 University of Washington, Seattle, WA 98195</footnote>

<footnote n="8"><sup>8</sup>United States Naval Observatory, 3450 Massachusetts Ave NW, Washington, D.C., 20392, USA</footnote>

<footnote n="9"><sup>9</sup>University of Wisconsin, Department of Astronomy, 475 N Charter St., Madison, WI 53706, USA</footnote>

<footnote>* E-mail: koch.eric.w@gmail.com (EWK); rosolowsky@ualberta.ca (EWR)</footnote>
<table><caption>**Table 1** Corrected version of Table C1. Circular rotation velocities were derived by DISKFIT (Sellwood & Spekkens 2015). The rotation model is fit to the peak velocity ($v_{peak}$) surface of the VLA+GBT data.</caption><thead><tr><th>Radius (")</th><th>Circ. Velocity (km s<sup>-1</sup>)</th></tr></thead><tbody><tr><td>9</td><td>1.58 ± 6.24</td></tr><tr><td>27</td><td>11.88 ± 5.26</td></tr><tr><td>45</td><td>22.71 ± 5.25</td></tr><tr><td>63</td><td>30.53 ± 5.12</td></tr><tr><td>81</td><td>29.95 ± 4.47</td></tr><tr><td>99</td><td>34.20 ± 4.03</td></tr><tr><td>117</td><td>36.76 ± 3.99</td></tr><tr><td>135</td><td>44.61 ± 3.79</td></tr><tr><td>153</td><td>47.80 ± 3.49</td></tr><tr><td>171</td><td>51.67 ± 3.08</td></tr><tr><td>189</td><td>52.73 ± 2.96</td></tr><tr><td>207</td><td>53.24 ± 3.06</td></tr><tr><td>225</td><td>55.30 ± 3.22</td></tr><tr><td>243</td><td>57.58 ± 3.30</td></tr><tr><td>261</td><td>58.70 ± 3.42</td></tr><tr><td>279</td><td>59.47 ± 3.50</td></tr><tr><td>297</td><td>60.30 ± 3.59</td></tr><tr><td>315</td><td>64.32 ± 3.78</td></tr><tr><td>333</td><td>67.66 ± 3.75</td></tr><tr><td>351</td><td>69.07 ± 4.03</td></tr><tr><td>369</td><td>72.05 ± 4.49</td></tr><tr><td>387</td><td>75.89 ± 4.82</td></tr><tr><td>405</td><td>74.09 ± 4.91</td></tr><tr><td>423</td><td>73.44 ± 3.29</td></tr><tr><td>441</td><td>77.06 ± 2.76</td></tr><tr><td>459</td><td>77.06 ± 2.80</td></tr><tr><td>477</td><td>77.82 ± 2.60</td></tr><tr><td>495</td><td>79.01 ± 2.48</td></tr><tr><td>513</td><td>80.96 ± 2.59</td></tr><tr><td>531</td><td>80.34 ± 2.50</td></tr><tr><td>549</td><td>80.35 ± 2.65</td></tr><tr><td>567</td><td>82.90 ± 2.66</td></tr><tr><td>585</td><td>86.23 ± 2.66</td></tr><tr><td>603</td><td>86.92 ± 2.59</td></tr><tr><td>621</td><td>86.13 ± 2.63</td></tr><tr><td>639</td><td>87.43 ± 2.57</td></tr><tr><td>657</td><td>87.89 ± 2.63</td></tr><tr><td>675</td><td>87.82 ± 2.35</td></tr><tr><td>693</td><td>91.08 ± 2.44</td></tr><tr><td>711</td><td>90.37 ± 2.25</td></tr><tr><td>729</td><td>88.22 ± 2.09</td></tr><tr><td>747</td><td>90.67 ± 2.36</td></tr><tr><td>765</td><td>92.32 ± 2.48</td></tr><tr><td>783</td><td>93.31 ± 2.26</td></tr><tr><td>801</td><td>94.15 ± 2.15</td></tr><tr><td>819</td><td>93.40 ± 2.37</td></tr><tr><td>837</td><td>94.02 ± 2.44</td></tr><tr><td>855</td><td>94.91 ± 2.50</td></tr><tr><td>873</td><td>95.57 ± 2.48</td></tr><tr><td>891</td><td>95.15 ± 2.22</td></tr><tr><td>909</td><td>93.19 ± 2.46</td></tr><tr><td>927</td><td>94.52 ± 2.63</td></tr><tr><td>945</td><td>95.00 ± 2.77</td></tr><tr><td>963</td><td>95.72 ± 2.90</td></tr><tr><td>981</td><td>96.89 ± 2.81</td></tr><tr><td>999</td><td>98.58 ± 2.73</td></tr><tr><td>1017</td><td>98.09 ± 2.61</td></tr><tr><td>1035</td><td>99.87 ± 2.53</td></tr><tr><td>1053</td><td>99.10 ± 2.41</td></tr><tr><td>1071</td><td>99.01 ± 2.40</td></tr><tr><td>1089</td><td>97.58 ± 2.21</td></tr><tr><td>1107</td><td>98.60 ± 2.26</td></tr><tr><td>1125</td><td>99.61 ± 2.22</td></tr></tbody></table>

<table><caption>**Table 1** – continued</caption><thead><tr><th>Radius (")</th><th>Circ. Velocity (km s<sup>-1</sup>)</th></tr></thead><tbody><tr><td>1143</td><td>99.61 ± 2.49</td></tr><tr><td>1161</td><td>102.02 ± 2.40</td></tr><tr><td>1179</td><td>101.84 ± 2.52</td></tr><tr><td>1197</td><td>102.76 ± 2.38</td></tr><tr><td>1215</td><td>102.66 ± 2.62</td></tr><tr><td>1233</td><td>102.57 ± 2.68</td></tr><tr><td>1251</td><td>104.08 ± 2.58</td></tr><tr><td>1269</td><td>103.24 ± 2.39</td></tr><tr><td>1287</td><td>103.17 ± 2.42</td></tr><tr><td>1305</td><td>103.33 ± 2.50</td></tr><tr><td>1323</td><td>103.41 ± 2.64</td></tr><tr><td>1341</td><td>103.91 ± 2.56</td></tr><tr><td>1359</td><td>102.91 ± 2.63</td></tr><tr><td>1377</td><td>105.50 ± 2.47</td></tr><tr><td>1395</td><td>104.05 ± 2.47</td></tr><tr><td>1413</td><td>106.03 ± 2.47</td></tr><tr><td>1431</td><td>104.89 ± 2.57</td></tr><tr><td>1449</td><td>106.68 ± 2.48</td></tr><tr><td>1467</td><td>105.53 ± 2.36</td></tr><tr><td>1485</td><td>105.80 ± 2.33</td></tr><tr><td>1503</td><td>104.03 ± 2.23</td></tr><tr><td>1521</td><td>105.58 ± 2.23</td></tr><tr><td>1539</td><td>105.69 ± 2.26</td></tr><tr><td>1557</td><td>106.32 ± 2.17</td></tr><tr><td>1575</td><td>105.97 ± 2.32</td></tr><tr><td>1593</td><td>105.58 ± 2.20</td></tr><tr><td>1611</td><td>106.18 ± 2.26</td></tr><tr><td>1629</td><td>106.08 ± 2.28</td></tr><tr><td>1647</td><td>106.24 ± 2.36</td></tr><tr><td>1665</td><td>106.39 ± 2.37</td></tr><tr><td>1683</td><td>106.47 ± 2.43</td></tr><tr><td>1701</td><td>107.19 ± 2.44</td></tr><tr><td>1719</td><td>105.88 ± 2.58</td></tr><tr><td>1737</td><td>106.58 ± 2.52</td></tr><tr><td>1755</td><td>106.09 ± 2.56</td></tr><tr><td>1773</td><td>106.30 ± 2.35</td></tr><tr><td>1791</td><td>107.23 ± 2.61</td></tr><tr><td>1809</td><td>104.01 ± 2.82</td></tr><tr><td>1827</td><td>104.50 ± 2.59</td></tr></tbody></table>

REFERENCE

Sellwood J. A., Spekkens K., 2015, preprint (arXiv:e-prints)

This paper has been typeset from a TeX/LA TeX file prepared by the author.