22 citations · 42 across the 8 of their papers we have counts for
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astro-ph.GA2026
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference
Scott Hagen, Carina Fian
Quasar microlensing is uniquely sensitive to the size-scale of the accretion flow, offering one of the few direct probes of the accretion structure on micro-arcsecond scales. Howev…
astro-ph.GA2017★ 22 cited
Boxy Orbital Structures in Rotating Bar Models
L. Chaves-Velasquez, P. A. Patsis, I. Puerari +2
We investigate regular and chaotic two-dimensional (2D) and three-dimensional (3D) orbits of stars in models of a galactic potential consisting in a disk, a halo and a bar, to find…