Cite
Inner mean-motion resonances with eccentric planets: a possible origin for exozodiacal dust clouds.
MLA
Faramaz, V., et al. “Inner Mean-Motion Resonances with Eccentric Planets: A Possible Origin for Exozodiacal Dust Clouds.” Monthly Notices of the Royal Astronomical Society, vol. 465, no. 2, Feb. 2017, pp. 2352–65. EBSCOhost, https://doi.org/10.1093/mnras/stw2846.
APA
Faramaz, V., Ertel, S., Booth, M., Cuadra, J., & Simmonds, C. (2017). Inner mean-motion resonances with eccentric planets: a possible origin for exozodiacal dust clouds. Monthly Notices of the Royal Astronomical Society, 465(2), 2352–2365. https://doi.org/10.1093/mnras/stw2846
Chicago
Faramaz, V., S. Ertel, M. Booth, J. Cuadra, and C. Simmonds. 2017. “Inner Mean-Motion Resonances with Eccentric Planets: A Possible Origin for Exozodiacal Dust Clouds.” Monthly Notices of the Royal Astronomical Society 465 (2): 2352–65. doi:10.1093/mnras/stw2846.