Microlensing of strongly lensed quasars

G Vernardos, D Sluse, D Pooley, RW Schmidt… - Space Science …, 2024 - Springer
Strong gravitational lensing of quasars has the potential to unlock the poorly understood
physics of these fascinating objects, as well as serve as a probe of the lensing mass …

Spatially resolved rotation of the broad-line region of a quasar at sub-parsec scale

Nature, 2018 - nature.com
The broadening of atomic emission lines by high-velocity motion of gas near accreting
supermassive black holes is an observational hallmark of quasars. Observations of broad …

High Eddington quasars as discovery tools: Current state and challenges

S Panda, P Marziani - Frontiers in Astronomy and Space Sciences, 2023 - frontiersin.org
A landmark of accretion processes in active galactic nuclei (AGN) is the continuum
originating from a complex structure, ie, an accretion disk and a corona around a …

A global view of the inner accretion and ejection flow around super massive black holes-Radiation-driven accretion disk winds in a physical context

M Giustini, D Proga - Astronomy & Astrophysics, 2019 - aanda.org
Context. Understanding the physics and geometry of accretion and ejection around super
massive black holes (SMBHs) is important to understand the evolution of active galactic …

Dust inflated accretion disc as the origin of the broad line region in active galactic nuclei

A Baskin, A Laor - Monthly Notices of the Royal Astronomical …, 2018 - academic.oup.com
The broad line region (BLR) in active galactic nuclei (AGNs) is composed of dense gas (∼
1011 cm− 3) on sub-pc scale, which absorbs about 30 per cent of the ionizing continuum …

In Situ Star Formation in Accretion Disks and Explanation of Correlation between the Black Hole Mass and Metallicity in Active Galactic Nuclei

X Fan, Q Wu - The Astrophysical Journal, 2023 - iopscience.iop.org
Recent observations show that the metallicity Z BLR of the broad-line region (BLR) in active
galactic nuclei (AGNs) is solar to supersolar, which is positively correlated with the mass of …

Direct evidence of non-disk optical continuum emission around an active black hole

D Chelouche, F Pozo Nuñez, S Kaspi - Nature Astronomy, 2019 - nature.com
Accretion onto black holes is key to their growth over cosmic time, especially during the
active galactic nuclei phase when the inflowing material forms a radiatively efficient …

Modeling of the quasar main sequence in the optical plane

S Panda, B Czerny, TP Adhikari… - The Astrophysical …, 2018 - iopscience.iop.org
The concept of the quasar main sequence is very attractive since it stresses correlations
between various parameters and implies the underlying simplicity. In the optical plane …

Expectations for time-delay measurements in active galactic nuclei with the Vera Rubin Observatory

B Czerny, S Panda, R Prince, VK Jaiswal… - Astronomy & …, 2023 - aanda.org
Context. The Vera Rubin Observatory will provide an unprecedented set of time-dependent
observations of the sky. The planned Legacy Survey of Space and Time (LSST), operating …

Can reverberation-measured quasars be used for cosmology?

ML Martínez-Aldama, B Czerny, D Kawka… - The Astrophysical …, 2019 - iopscience.iop.org
Quasars have been proposed as a new class of standard candles analogous to supernovae,
since their large redshift range and high luminosities make them excellent candidates. The …