Issue |
A&A
Volume 693, January 2025
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 1 | |
Section | Galactic structure, stellar clusters and populations | |
DOI | https://doi.org/10.1051/0004-6361/202348837e | |
Published online | 24 December 2024 |
The e-TidalGCs project
Modeling the extra-tidal features generated by Galactic globular clusters (Corrigendum)
1
GEPI, Observatoire de Paris, PSL Research University, CNRS, Place Jules Janssen, 92195 Meudon Cedex, France
e-mail: salvatore.ferrone@obspm.fr
2
SMC-ISC-CNR and Dipartimento di Fisica, Sapienza University, P.le Aldo Moro 2, 00185 Rome, Italy
3
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
4
LERMA, CNRS UMR 8122, Observatoire de Paris, PSL, 61 Avenue de l’Observatoire, 75014 Paris, France
Received:
4
December
2023
Accepted:
13
December
2023
Key words: globular clusters: general / Galaxy: structure / Galaxy: kinematics and dynamics / Galaxy: evolution / methods: numerical / errata, addenda
In the initial version of the paper, there was a minor error in Eq. (6), where the first term inaccurately used Mhalo instead of the correct expression, Mhalo(r). This correction specifies the halo mass enclosed at the galactocentric radius, r, rather than the total mass. Importantly, this correction is confined to the equation’s presentation in the text and does not impact the accuracy of the results presented in the original paper. The computations were conducted using the accurate expression, ensuring the integrity of the findings. The correct equation is as follows:
where Mhalo is the total mass of the halo and Mhalo(r) is the enclosed halo mass at radius r from the galactic center. Also, ahalo is the characteristic scale length.
© The Authors 2024
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