Aberration effect on lower-order images of a thin accretion disk in the astrometric approach

Zhu, Qing-Hua

doi:10.1103/physrevd.109.044057

Cited by 1 publication

(1 citation statement)

References 43 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…In the field of theoretical research, many previous studies mainly focus on the gravitational lensing effect stemming from spacetime geometry, where the light sources are modeled to be of simple structures and often as geometrically thin disks [15][16][17][18][19][20][21][22][23][24][25][26][27][28][29][30][31][32][33]. However, for a low-luminosity active galactic nuclei (LLAGN) like the M87*, the horizon-scale accretion flow is mostly geometrically thick [2,34].…”

Section: Introductionmentioning

confidence: 99%

Imaging thick accretion disks and jets surrounding black holes

Zhang,

Hou,

Guo

et al. 2024

J. Cosmol. Astropart. Phys.

View full text Add to dashboard Cite

Based on the horizon-scale magnetofluid model developed in [1], we investigate the millimeter-wave images of a geometrically thick accretion disk or a funnel wall, i.e., the magnetofluid that encloses the base of the jet region, around a Kerr black hole. By employing the numerical method to solve the null geodesic and radiative transfer equations, we obtain the optical appearances at various observational angles and frequencies, generated by the thermal synchrotron radiation within the magnetofluid. For the thick disk, we specifically examine the impact of emission anisotropy on images, concluding that anisotropic synchrotron radiation could play an important role in the observability of the photon ring. For the funnel wall, we find that both the outflow and inflow funnel walls exhibit annular structures on the imaging plane. The outflow funnel wall yields a brighter primary image than the photon ring, whereas the inflow one does not. Based on our investigation, the inflow funnel wall model can not be ruled out by current observations of M87*.

show abstract