APA (7th ed.) Citation

Caussi, M. L., Dombard, A. J., Korycansky, D. G., White, O. L., Moore, J. M., & Schenk, P. M. (2024). Dome Craters on Ganymede and Callisto May Form by Topographic Relaxation of Pit Craters Aided by Remnant Impact Heat.

Chicago Style (17th ed.) Citation

Caussi, Martina L., Andrew J. Dombard, Donald G. Korycansky, Oliver L. White, Jeffrey M. Moore, and Paul M. Schenk. Dome Craters on Ganymede and Callisto May Form by Topographic Relaxation of Pit Craters Aided by Remnant Impact Heat. 2024.

MLA (9th ed.) Citation

Caussi, Martina L., et al. Dome Craters on Ganymede and Callisto May Form by Topographic Relaxation of Pit Craters Aided by Remnant Impact Heat. 2024.