Erratum: “Resolved Nuclear Kinematics Link the
Formation and Growth of Nuclear Star Clusters with
the Evolution of Their Early and Late-type Hosts”
(2021, ApJ, 921, 8)

Francesca Pinna, Nadine Neumayer, Anil Seth, Eric Emsellem, Dieu Nguyen, Torsten Böker, Michele Cappellari, Richard Mcdermid, Karina Voggel, C.

Jakob Walcher

► To cite this version:

Francesca Pinna, Nadine Neumayer, Anil Seth, Eric Emsellem, Dieu Nguyen, et al. Erratum: “Resolved Nuclear Kinematics Link the Formation and Growth of Nuclear Star Clusters with the Evolution of Their Early and Late-type Hosts” (2021, ApJ, 921, 8). The Astrophysical Journal, 2021, 923 (2), pp.283. 10.3847/1538-4357/ac4011. hal-03509454

HAL Id: hal-03509454

https://hal.science/hal-03509454v1

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Distributed under a Creative Commons Attribution 4.0 International License
Erratum: “Resolved Nuclear Kinematics Link the Formation and Growth of Nuclear Star Clusters with the Evolution of Their Early and Late-type Hosts” (2021, ApJ, 921, 8)

Francesca Pinna¹, Nadine Neumayer¹, Anil Seth², Eric Emsellem³, Dieu D. Nguyen⁴, Torsten Böker⁵, Michele Cappellari⁶, Richard M. McDermid⁷, Karina Voggel⁸, and C. Jakob Walcher⁹

¹Max Planck Institute for Astronomy, D-69117 Heidelberg, Germany; pinna@mpia.de

²Department of Physics and Astronomy, University of Utah, UT 84112, USA

³European Southern Observatory, D-85748 Garching bei Muenchen, Germany

⁴National Astronomical Observatory of Japan (NAOJ), National Institute of Natural Sciences (NINS), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

⁵European Space Agency/STScI, Baltimore, MD 21218, USA

⁶Department of Physics, University of Oxford, OX1 3RH, UK

⁷Research Centre for Astronomy, Astrophysics, and Astrophotonics, Macquarie University, Sydney, NSW 2109, Australia

⁸Université de Strasbourg, CNRS, Observatoire astronomique de Strasbourg, UMR 7550, F-67000 Strasbourg, France

⁹Leibniz-Institut für Astrophysik Potsdam (AIP) D-14482 Potsdam, Germany

Received 2021 December 2; published 2021 December 29

We have identified an error in Equations (D3) and (D4) in Appendix D of the published article. These equations result from the combination of Equations (16), (17), and (18) in Harborne et al. (2020). In the published article, the right-hand sides are swapped with each other. The corrected versions of the equations are

$$ \Delta\left(\frac{V}{\sigma}\right)_e^{\text{corr}} = \left\{ \frac{7.55}{1 + \exp\left[4.42\left(\frac{\sigma_{\text{PSF}}}{R_e^{\text{maj}}}\right)^{1.55} + 2.73\right]} - 0.46 \right\} + 3\left(\frac{\sigma_{\text{PSF}}}{R_e^{\text{maj}}}\right) \times [-0.10\epsilon_e + 0.024\log_{10}(n_{\text{NSC}}) + 0.064] \quad (D3) $$

and

$$ \Delta\lambda_{R_e}^{\text{corr}} = \left\{ \frac{7.48}{1 + \exp\left[4.08\left(\frac{\sigma_{\text{PSF}}}{R_e^{\text{maj}}}\right)^{1.60} + 2.89\right]} - 0.39 \right\} + \left(\frac{\sigma_{\text{PSF}}}{R_e^{\text{maj}}}\right) \times [0.10\epsilon_e - 0.22\log_{10}(n_{\text{NSC}}) + 0.10]. \quad (D4) $$

All results shown and discussed in the published article were obtained using the correct version of the equations and do not need any modifications.

ORCID iDs

Francesca Pinna https://orcid.org/0000-0001-5965-3530

Nadine Neumayer https://orcid.org/0000-0002-6922-2598

Anil Seth https://orcid.org/0000-0003-0248-5470

Eric Emsellem https://orcid.org/0000-0002-6155-7166

Dieu D. Nguyen https://orcid.org/0000-0002-5678-1008

Torsten Böker https://orcid.org/0000-0002-5666-7782

Michele Cappellari https://orcid.org/0000-0002-1283-8420

Richard M. McDermid https://orcid.org/0000-0002-8175-7229

Karina Voggel https://orcid.org/0000-0001-6215-0950

C. Jakob Walcher https://orcid.org/0000-0002-2715-796X

References

Harborne, K. E., van de Sande, J., Cortese, L., et al. 2020, MNRAS, 497, 2018

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