Schwarzschild modelling of barred s0 galaxy NGC 4371
We apply the barred Schwarzschild method developed by Tahmasebzadeh et al. (2022) to a barred S0 galaxy, NGC 4371, observed by IFU instruments from the TIMER and ATLAS3D projects. We construct the gravitational potential by combining a fixed black hole mass, a spherical dark matter halo, and stellar mass distribution deprojected from 3.6 μm S $^4$G
Tahmasebzadeh, Behzad et al.
Fecha de publicación:
10
2024