activity
20182024
most citedDiscovery of a hot ultramassive rapidly rotating DBA White Dwarf

39 citations · 69 across the 8 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2024

Detection of Gamma-ray Halos around Nearby Late-type Galaxies

M. S. Pshirkov, B. A. Nizamov

Various theoretical models predict the existence of extended -ray halo around normal galaxies that could be produced by interactions of cosmic rays with the circumgalactic mediu…

astro-ph.HE2024

Annihilation of positrons from AGN jets as a possible source of cosmic gamma-ray background at energies below 511 keV

B. A. Nizamov, M. S. Pshirkov

The origin of the diffuse gamma-ray background in the range from hundreds keV to several MeV is not known conclusively. From current models and observations it is believed that, at…

astro-ph.HE2023★ 14 cited

Can observations of 511 keV line from the M31 galaxy shed light on the AGN jet composition?

B. A. Nizamov, M. S. Pshirkov

Positron annihilation line at 511~keV is a known component of the gamma-ray diffuse emission. It is believed to be produced in the Galaxy, but there could be possible extragalactic…

astro-ph.HE2022★ 1 cited

Gamma-ray flares from pulsar wind nebulae in the Large Magellanic Cloud

B. A. Nizamov, M. S. Pshirkov

High-energy radiation of young pulsar wind nebulae (PWNe) is known to be variable. This is most prominently exemplified by the Crab nebula which can undergo both rapid brightenings…

astro-ph.HE2020★ 11 cited

Gamma-ray flux depressions of the Crab nebula in the high-energy range

M. S. Pshirkov, B. A. Nizamov, A. M. Bykov +1

The giant gamma-ray flares of the Crab nebula discovered by AGILE and Fermi observatories came as a surprise and have challenged the existing models of pulsar wind nebulae. We have…

astro-ph.HE2018★ 2 cited

Constraints on the AGN flares as sources of ultra-high energy cosmic rays from the Fermi-LAT observations

B. A. Nizamov, M. S. Pshirkov

It is well known that if the most energetic cosmic rays ( eV) were protons then their acceleration sites should possess some extreme properties, including gigantic lumin…