Rotation curves and dynamical masses of MaNGA barred galaxies

Schmidt, Eduardo O.; Mast, Damián; Gaspar, Gaia; Weidmann, Walter

doi:10.1093/mnras/stad1531

Rotation curves and dynamical masses of MaNGA barred galaxies

Journal Article · Fri May 19 00:00:00 EDT 2023 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stad1531· OSTI ID:1975917

Schmidt, Eduardo O. ^[1]; Mast, Damián ^[1]; Gaspar, Gaia ^[1]; Weidmann, Walter ^[1]

Universidad Nacional de Córdoba (Argentina); Consejo de Investigaciones Científicas y Técnicas de la República Argentina (CONICET), Buenos Aires (Argentina)

In this paper we analyse a sample of 46 barred galaxies of MaNGA. Our goal is to investigate the stellar kinematics of these galaxies and obtain their rotation curves. Additionally, we aim to derive the total stellar and dynamical masses, as well as the maximum rotation velocity, in order to examine their distributions and scaling relations. Using the Pipe3D dataproducts publicly available we obtained the rotation curves, which were fitted considering two components of an axisymmetric Miyamoto–Nagai gravitational potential. We found a wide range of the maximum rotation velocities (117–340 $${\rm km\, s^{-1}}$$), with a mean value of 200 $${\rm km\, s^{-1}}$$. In addition we found that the total stellar and dynamical masses are in the range of log(M_star/M_⊙) = 10.1−11.5, with a mean value of log(M_star/M_⊙) = 10.8, and log(M_dyn/M_⊙) = 10.4−12.0, with a mean value of log(M_dyn/M_⊙) = 11.1, respectively. We found a strong correlation between dynamical mass and maximum velocity, between maximum velocity and magnitude, and between stellar mass and maximum velocity. According to these results, barred galaxies exhibit similar behaviour to that of normal spiral galaxies with respect to these relations, as well as in terms of the distribution of their dynamical mass and maximum rotation velocity. However, we found that the distribution of stellar masses of barred galaxies is statistically different from other samples including non-barred galaxies. Finally, analysing the galaxies that show nuclear activity, we find no difference with the rotation curves of normal galaxies.

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Research Organization:: US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)

Sponsoring Organization:: Fondo para la Investigación Científica y Tecnológica (FonCyT); USDOE; USDOE Office of Science (SC)

OSTI ID:: 1975917

Alternate ID(s):: OSTI ID: 2425272

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 523; ISSN 0035-8711; ISSN 1365-2966

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United States

Language:: English

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