A method for selecting M dwarfs with an increased likelihood of unresolved ultracool companionship.

MLA

Cook, N. J., et al. “A Method for Selecting M Dwarfs with an Increased Likelihood of Unresolved Ultracool Companionship.” Monthly Notices of the Royal Astronomical Society, vol. 457, no. 2, Apr. 2016, pp. 2192–208. EBSCOhost, https://doi.org/10.1093/mnras/stw061.

APA

Cook, N. J., Pinfield, D. J., Marocco, F., Burningham, B., Jones, H. R. A., Frith, J., Zhong, J., Luo, A. L., Qi, Z. X., Lucas, P. W., Gromadzki, M., Day-Jones, A. C., Kurtev, R. G., Guo, Y. X., Wang, Y. F., Bai, Y., Yi, Z. P., & Smart, R. L. (2016). A method for selecting M dwarfs with an increased likelihood of unresolved ultracool companionship. Monthly Notices of the Royal Astronomical Society, 457(2), 2192–2208. https://doi.org/10.1093/mnras/stw061

Chicago

Cook, N. J., D. J. Pinfield, F. Marocco, B. Burningham, H. R. A. Jones, J. Frith, J. Zhong, et al. 2016. “A Method for Selecting M Dwarfs with an Increased Likelihood of Unresolved Ultracool Companionship.” Monthly Notices of the Royal Astronomical Society 457 (2): 2192–2208. doi:10.1093/mnras/stw061.