SDSS-IV MaNGA: spatial resolved properties of kinematically misaligned galaxies

Xu, Haitong; Chen, Yanmei; Shi, Yong; Zhou, Yuren; Bizyaev, Dmitry; Bao, Min; Beom, Minje; Fernández-Trincado, José G.; Cao, Xiao

doi:10.1093/mnras/stac354

Title: SDSS-IV MaNGA: spatial resolved properties of kinematically misaligned galaxies

Journal Article · 10 February 2022 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stac354 · OSTI ID:1982669

Xu, Haitong ^[1]; Chen, Yanmei ^[1];

^[1];

^[2]; Bao, Min ^[1]; Beom, Minje ^[3]; Fernández-Trincado, José G. ^[4]; Cao, Xiao ^[1]

Nanjing University (China); Collaborative Innovation Center of Modern Astronomy and Space Exploration, Nanjing (China)
Apache Point Observatory and New Mexico State University, Sunspot, NM (United States); Moscow State University (Russia)
New Mexico State University, Las Cruces, NM (United States)
Universidad Católica del Norte, Antofagasta (Chile); Universidad de Atacama, Copiapó (Chile)

We select 456 galaxies with kinematically misaligned gas and stellar components from 9456 parent galaxies in MaNGA, and classify them into 72 star-forming galaxies, 142 green-valley galaxies, and 242 quiescent galaxies. Comparing the spatial resolved properties of the misaligned galaxies with control samples closely match in the Dn4000 and stellar velocity dispersion, we find that: (1) the misaligned galaxies have lower values in V_gas/σ_gas and V_star/σ_star (the ratio between ordered to random motion of gas and stellar components) across the entire galaxies than their control samples; (2) the star-forming and green-valley misaligned galaxies have enhanced central concentrated star formation than their control galaxies. The difference in stellar population between quiescent misaligned galaxies and control samples is small; (3) gas-phase metallicity of the green valley and quiescent misaligned galaxies are lower than the control samples. For the star-forming misaligned galaxies, the difference in metallicity between the misaligned galaxies and their control samples strongly depends on how we select the control samples. All these observational results suggest that external gas accretion influences the evolution of star forming and green-valley galaxies, not only in kinematics/morphologies, but also in stellar populations. Furthermore, the quiescent misaligned galaxies have survived from different formation mechanisms.

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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:: USDOE

OSTI ID:: 1982669

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 4 Vol. 511; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United States

Language:: English

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