Open Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202244141]


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

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:

Φ halo ( r ) = G M halo ( r ) r M halo 1.02 a halo × [ 1.02 1 + ( r a halo ) 1.02 + ln ( 1 + ( r a halo ) 1.02 ) ] R 100 , $$ \begin{aligned} \Phi _{\rm halo}(r) =&\frac{-GM_{\rm halo}(r)}{r} -\frac{M_{\rm halo}}{1.02a_{\rm halo}}\\&\times \left[\frac{-1.02}{1+\left(\frac{r}{a_{\rm halo}}\right)^{1.02}}+\ln {\left(1+\left(\frac{r}{a_{\rm halo}}\right)^{1.02}\right)}\right]_R^{100}, \end{aligned} $$

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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