SDSS-IV MaNGA: Stellar population correlates with stellar root-mean-square velocity $V_{\rm rms}$ gradients or total-density-profile slopes at fixed effective velocity dispersion $\sigma_{\rm e}$

MLA

Lu, Shengdong, et al. SDSS-IV MaNGA: Stellar Population Correlates with Stellar Root-Mean-Square Velocity $V_{\rm Rms}$ Gradients or Total-Density-Profile Slopes at Fixed Effective Velocity Dispersion $\sigma_{\rm E}$. 2020. EBSCOhost, https://doi.org/10.1093/mnras/staa1481.

APA

Lu, S., Cappellari, M., Mao, S., Ge, J., & Li, R. (2020). SDSS-IV MaNGA: Stellar population correlates with stellar root-mean-square velocity $V_{\rm rms}$ gradients or total-density-profile slopes at fixed effective velocity dispersion $\sigma_{\rm e}$. https://doi.org/10.1093/mnras/staa1481

Chicago

Lu, Shengdong, Michele Cappellari, Shude Mao, Junqiang Ge, and Ran Li. 2020. “SDSS-IV MaNGA: Stellar Population Correlates with Stellar Root-Mean-Square Velocity $V_{\rm Rms}$ Gradients or Total-Density-Profile Slopes at Fixed Effective Velocity Dispersion $\sigma_{\rm E}$.” doi:10.1093/mnras/staa1481.