NIHAO XXIV: rotation- or pressure-supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics.

MLA

Cardona-Barrero, Salvador, et al. “NIHAO XXIV: Rotation- or Pressure-Supported Systems? Simulated Ultra Diffuse Galaxies Show a Broad Distribution in Their Stellar Kinematics.” Monthly Notices of the Royal Astronomical Society, vol. 497, no. 4, Oct. 2020, pp. 4282–92. EBSCOhost, https://doi.org/10.1093/mnras/staa2094.

APA

Cardona-Barrero, S., Di, C. A., Brook, C. B. A., Ruiz-Lara, T., Beasley, M. A., Falcón-Barroso, J., & Macciò, A. V. (2020). NIHAO XXIV: rotation- or pressure-supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics. Monthly Notices of the Royal Astronomical Society, 497(4), 4282–4292. https://doi.org/10.1093/mnras/staa2094

Chicago

Cardona-Barrero, Salvador, Cintio, Arianna Di, Christopher B A Brook, Tomas Ruiz-Lara, Michael A Beasley, Jesus Falcón-Barroso, and Andrea V Macciò. 2020. “NIHAO XXIV: Rotation- or Pressure-Supported Systems? Simulated Ultra Diffuse Galaxies Show a Broad Distribution in Their Stellar Kinematics.” Monthly Notices of the Royal Astronomical Society 497 (4): 4282–92. doi:10.1093/mnras/staa2094.