Open Access

Table 1.

Main properties of NGC 1427A.

IDs NGC 1427A, ESO 358-G049, FCC 235
RA (J2000) (1) 3h 40m 8.7s This work
Dec (J2000) (1) −35d 37m 34s This work
vsys(1) 2036 km s −1 This work
Distance (2) 20 Mpc Tonry et al. (2001)
M (2.3 ± 0.5)×109 M Loni et al. (2021)
MHI(3) (2.3 ± 0.2)×109 M This work

Notes. (1) The central coordinates and systemic velocity are those of the dynamical centre (Sect. 3.2). Throughout this paper we list barycentric velocities in the optical convention v = c × (ν0/ν − 1), where c is the speed of light, ν0 the rest frequency, and ν the observed frequency in the barycentric frame of reference. (2) This is the distance of the Fornax cluster as a whole. (3) The value reported here for the H I mass is measured from the image at 66″ resolution, while at higher resolution it is slightly lower. The uncertainty is calculated by adding in quadrature the statistical uncertainty within the H I detection mask (which depends on the noise level in the cube and the number of independent voxels in the mask) and a 10% flux scale uncertainty (Serra et al. 2023). The latter term dominates the error budget.

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