Cosmological simulations with self-interacting dark matter – II. Halo shapes versus observations.

MLA

Peter, Annika H. G., et al. “Cosmological Simulations with Self-Interacting Dark Matter – II. Halo Shapes versus Observations.” Monthly Notices of the Royal Astronomical Society, vol. 430, no. 1, Mar. 2013, pp. 105–20. EBSCOhost, https://doi.org/10.1093/mnras/sts535.

APA

Peter, A. H. G., Rocha, M., Bullock, J. S., & Kaplinghat, M. (2013). Cosmological simulations with self-interacting dark matter – II. Halo shapes versus observations. Monthly Notices of the Royal Astronomical Society, 430(1), 105–120. https://doi.org/10.1093/mnras/sts535

Chicago

Peter, Annika H. G., Miguel Rocha, James S. Bullock, and Manoj Kaplinghat. 2013. “Cosmological Simulations with Self-Interacting Dark Matter – II. Halo Shapes versus Observations.” Monthly Notices of the Royal Astronomical Society 430 (1): 105–20. doi:10.1093/mnras/sts535.