activity
20032026
most citedMagnetic Fields of Agns and Standard Accretion Disk Model: Testing by Optical Polarimetry

43 citations · 214 across the 35 of their papers we have counts for

collaborators

36 papers

astro-ph.HE2026

Disk-Like Matter Outflow from a Kerr-Type Wormhole: Possible Observational Manifestations and Magnetic Effects

Mikhail Piotrovich, Stanislava Buliga, Tinatin Natsvlishvili

We present a phenomenological study of a hypothetical compact object with a traversable 2 Kerr-type wormhole geometry connecting two asymptotically distinct regions. One mouth of t…

astro-ph.HE2026

Estimation of black hole spins in low-mass AGNs and comparison with other types of AGNs

M. Yu. Piotrovich, S. D. Buliga, T. M. Natsvlishvili

We estimated the spins of a sample of 58 low-mass AGNs. Analysis of the obtained spins showed that they decrease with increasing SMBH mass, leading us to hypothesize that mergers a…

astro-ph.HE2026

Red Quasars: Selecting Candidates in SDSS DR16 and Estimating Their Physical Parameters

M. Yu. Piotrovich, S. D. Buliga, T. M. Natsvlishvili

Using ''color cut'' method we obtained from SDSS DR16 catalog 733 red quasar candidates which amounted to approximately 4% of the objects from the initial sample. Then we estimated…

astro-ph.HE2025★ 1 cited

Spins of SMBHs in distant low luminosity AGNs

M. Yu. Piotrovich, S. D. Buliga, T. M. Natsvlishvili

We estimated radiative efficiency, spin and SMBH mass values for sample of 33 distant low luminosity AGNs. The distribution of the estimated spin values (majority of objects have a…

astro-ph.HE2025★ 1 cited

MAD-Accretion Scenario in High-Mass X-Ray Binaries with Neutron Stars

N. R. Ikhsanov, M. Yu. Piotrovich, N. G. Beskrovnaya

The wind-fed accretion of gas with an intrinsic magnetic field onto neutron stars in high-mass X-ray binaries (HMXBs) is discussed. The criteria for the implementation of quasi-sph…

astro-ph.HE2025

Estimating the spins of supermassive black holes in distant ultraluminous quasars

M. Yu. Piotrovich, S. D. Buliga, T. M. Natsvlishvili

We estimated spin, inclination angle and corresponding SMBH mass values for sample of extremely distant (6 < z < 7.5) ultraluminous quasars. The estimated spin values are on averag…