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@article{2301502,
author = {Czerny, Bozena and Cao, Shulei and Jaiswal, Vikram Kumar and Karas, Vladimír and Khadka, Narayan and MartínezandAldama, Mary Loli and Naddaf, Mohammad Hassan and Panda, Swayamtrupta and Nuñez, Francisco Pozo and Prince, Raj and Ratra, Bharat and Sniegowska, Marzena and Yu, Zhefu and Zajaček, Michal},
article_number = {2},
doi = {http://dx.doi.org/10.1007/s10509-023-04165-7},
keywords = {Black holes; Galaxies; Accretion disks; Active galactic nuclei},
language = {eng},
issn = {0004-640X},
journal = {Astrophysics and Space Science},
title = {Accretion disks, quasars and cosmology: meandering towards understanding},
url = {https://doi.org/10.1007/s10509-023-04165-7},
volume = {368},
year = {2023}
}
TY - JOUR
ID - 2301502
AU - Czerny, Bozena - Cao, Shulei - Jaiswal, Vikram Kumar - Karas, Vladimír - Khadka, Narayan - Martínez-Aldama, Mary Loli - Naddaf, Mohammad Hassan - Panda, Swayamtrupta - Nuñez, Francisco Pozo - Prince, Raj - Ratra, Bharat - Sniegowska, Marzena - Yu, Zhefu - Zajaček, Michal
PY - 2023
TI - Accretion disks, quasars and cosmology: meandering towards understanding
JF - Astrophysics and Space Science
VL - 368
IS - 2
SP - 1-13
EP - 1-13
PB - Springer
SN - 0004640X
KW - Black holes
KW - Galaxies
KW - Accretion disks
KW - Active galactic nuclei
UR - https://doi.org/10.1007/s10509-023-04165-7
N2 - 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.
ER -
CZERNY, Bozena, 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 a Michal ZAJAČEK. Accretion disks, quasars and cosmology: meandering towards understanding. \textit{Astrophysics and Space Science}. Springer, 2023, roč.~368, č.~2, s.~1-13. ISSN~0004-640X. Dostupné z: https://dx.doi.org/10.1007/s10509-023-04165-7.
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