1. MaNGA DynPop – V. The dark-matter fraction versus stellar velocity dispersion relation and stellar initial mass function variations in galaxies: dynamical models and full spectrum fitting of integral-field spectroscopy.
- Author
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Lu, Shengdong, Zhu, Kai, Cappellari, Michele, Li, Ran, Mao, Shude, and Xu, Dandan
- Subjects
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DISPERSION relations , *STELLAR initial mass function , *GALAXIES , *GALAXY spectra , *STELLAR mass , *STELLAR populations - Abstract
Using the final Mapping Nearby Galaxies at Apache Point Observatory sample of 10K galaxies, we investigate the dark matter (DM) fraction f DM within one half-light radius R e for about 6K galaxies with good kinematics spanning a wide range of morphologies and stellar velocity dispersion. We employ two techniques to estimate f DM: (i) Jeans anisotropic modelling (JAM), which performs DM decomposition based on stellar kinematics and (ii) comparing the total dynamical mass-to-light ratios (M / L)JAM and (M */ L)SPS from stellar population synthesis (SPS). We find that both methods consistently show a significant trend of increasing f DM with decreasing σe and low f DM at larger σe. For 235 early-type galaxies with the best models, we explore the variation of stellar initial mass function (IMF) by comparing the stellar mass-to-light ratios from JAM and SPS. We confirm that the stellar mass excess factor αIMF increases with σe, consistent with previous studies that reported a transition from Chabrier-like to Salpeter IMF among galaxies. We show that the αIMF trend cannot be driven by M */ L or IMF gradients as it persists when allowing for radial gradients in our model. We find no evidence for the total M / L increasing toward the centre. We detect weak positive correlations between αIMF and age, but no correlations with metallicity. We stack galaxy spectra according to their αIMF to search for differences in IMF-sensitive spectral features (e.g. the |$\rm Na_{\rm I}$| doublet). We only find marginal evidence for such differences, which casts doubt on the validity of one or both methods to measure the IMF. [ABSTRACT FROM AUTHOR]
- Published
- 2024
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