Accretion disks, quasars and cosmology: meandering towards understanding

        As Setti and Woltjer noted back in 1973, one can use quasars to construct the Hubble diagram; however, the actual application of the idea was not that straightforward. It took years to implement the proposition successfully. Most ways to employ quasars for cosmology now require an advanced understanding of their structure, step by step. We briefly review this progress, with unavoidable personal biases, and concentrate on bright unobscured sources. We will mention the problem of the gas flow character close to the innermost stable circular orbit near the black hole, as discussed five decades ago. This problem later led to the development of the slim disk scenario and is recently revived in the context of Magnetically Arrested Disks (MAD) and Standard and Normal Evolution (SANE) models. We also discuss the hot or warm corona issue, which is still under debate and complicates the analysis of X-ray reflection. We present the scenario of the formation of the low ionization part of the Broad Line Region as a failed wind powered by radiation pressure acting on dust (Failed Radiatively Driven Dusty Outflow – FRADO). Next, we examine the cosmological constraints currently achievable with quasars, primarily concentrating on light echo methods (continuum time delays and spectral-line time delays to the continuum) that are (or should be) incorporating the progress mentioned above. Finally, we briefly discuss prospects in this lively subject area.


DOI: 10.1007/s10509-023-04165-7

Research Groups: Astroinformatics

Publication type: Journal

Journal: Astrophysics and Space Science

Citation: Astrophys Space Sci 368(2),8

Date Published: 1st Feb 2023

Registered Mode: by DOI

Authors: Bożena Czerny, Shulei Cao, Vikram Kumar Jaiswal, Vladimír Karas, Narayan Khadka, Mary Loli Martínez-Aldama, Mohammad Hassan Naddaf, Swayamtrupta Panda, Francisco Pozo Nuñez, Raj Prince, Bharat Ratra, Marzena Sniegowska, Zhefu Yu, Michal Zajaček

help Submitter
Czerny, B., Cao, S., Jaiswal, V. K., Karas, V., Khadka, N., Martínez-Aldama, M. L., Naddaf, M. H., Panda, S., Pozo Nuñez, F., Prince, R., Ratra, B., Sniegowska, M., Yu, Z., & Zajaček, M. (2023). Accretion disks, quasars and cosmology: meandering towards understanding. In Astrophysics and Space Science (Vol. 368, Issue 2). Springer Science and Business Media LLC.

Views: 1998

Created: 21st Feb 2023 at 07:23

Last updated: 5th Mar 2024 at 21:25

help Tags

This item has not yet been tagged.

help Attributions


Powered by
Copyright © 2008 - 2023 The University of Manchester and HITS gGmbH