APA (7th ed.) Citation

Stute, M., & Camenzind, M. (2002). Towards a self-consistent relativistic model of the exterior gravitational field of rapidly rotating neutron stars. Monthly notices of the Royal Astronomical Society, 336(3), 831-840. https://doi.org/10.1046/j.1365-8711.2002.05820.x

Chicago Style (17th ed.) Citation

Stute, Matthias, and Max Camenzind. "Towards a Self-consistent Relativistic Model of the Exterior Gravitational Field of Rapidly Rotating Neutron Stars." Monthly Notices of the Royal Astronomical Society 336, no. 3 (2002): 831-840. https://doi.org/10.1046/j.1365-8711.2002.05820.x.

MLA (9th ed.) Citation

Stute, Matthias, and Max Camenzind. "Towards a Self-consistent Relativistic Model of the Exterior Gravitational Field of Rapidly Rotating Neutron Stars." Monthly Notices of the Royal Astronomical Society, vol. 336, no. 3, 2002, pp. 831-840, https://doi.org/10.1046/j.1365-8711.2002.05820.x.