Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star
Authors: Slavko Bogdanov, Frederick K. Lamb, Simin Mahmoodifar, M. Coleman Miller, Sharon M. Morsink, Thomas E. Riley, Tod E. Strohmayer, Albert K. Tung, Anna L. Watts, Alexander J. Dittmann, Deepto Chakrabarty, Sebastien Guillot, Zaven Arzoumanian, and Keith C. Gendreau
2019 The Astrophysical Journal Letters887L26.
Provider: AAS Journals
Caption: Figure 7.
Same as Figure 5 but for comparisons of the synthetic pulse waveforms from Tests SD1e and SD1f, which consider a rapidly spinning (400 Hz) neutron star and more general combinations of colatitude and viewing angle.