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19912026
most citedPlanck 2015 results. XIII. Cosmological parameters

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283 papers · 1 filter

astro-ph.HE2026

Possible Sources of Iron Nuclei in Ultra-High-Energy Cosmic Rays

Anna Uryson

The origin of a cosmic ray particle with an ultra-high energy of 2.44 x 10^20 eV recorded by the Telescope Array is discussed by assuming that it is a heavy nucleus, namely an iron…

astro-ph.HE2026

A broadband outburst of the compact steep-spectrum quasar 3C 138 in 2024-2026

T. V. Mufakharov, Yu. V. Sotnikova, V. V. Vlasyuk +20

After several decades of relative quiescence, the compact steep-spectrum quasar 3C 138 entered an active phase in 2024-2026, exhibiting strong broadband flaring. We investigate its…

astro-ph.HE2026

Synchrotron radiation in nonuniform magnetic field

V. S. Beskin, A. Yu. Istomin, F. A. Kniazev +1

The distortion of the spectrum of synchrotron radiation received by a distant observer due to magnetic field inhomogeneity is discussed. It is shown that for single-particle radiat…

astro-ph.HE2026

Magnetic field and plasma number density from radio and millimeter core measurements in AGN jets

E. E. Nokhrina, A. P. Lobanov, A. Yu. Istomin +1

Understanding the mechanism for launching relativistic jets in active galactic nuclei relies upon measuring the magnetic field strength and emitting plasma number density, tracing…

astro-ph.HE2026

A hidden ultra-relativistic spine in the jet of a neutrino-associated blazar

Y. Y. Kovalev, F. Eppel, D. C. Homan +16

Supermassive black holes launch powerful jets of plasma that can accelerate particles to extreme energies, but the physical conditions required to produce high-energy neutrinos rem…

astro-ph.HE2026

Hydrodynamic model of nonthermal emission from the Fermi bubbles

V. A. Dogiel, D. O. Chernyshov, T. S. Fatekhov +2

We suggest a model of Fermi Bubbles (FBs) in the Galactic halo of the altitude about 7-8 kpc, which is seen in non-thermal microwave and gamma-ray ranges. It was assumed that this…

astro-ph.HE2026★ 1 cited

Multiwavelength quasi-periodic variability of the blazar Ton 599

Yu. V. Sotnikova, T. V. Mufakharov, A. E. Volvach +34

During the last 40-50 years, the TeV blazar Ton 599 has systematically experienced major outbursts detected in a wide wavelength range from radio to -rays. In this work, we pres…

astro-ph.HE2026

The nearby He-rich superluminous supernova SN 2021bnw during photospheric phases

A. Fiore, A. Kozyreva, L. Yan +40

Aim. We present and interpret the data of the nearby hydrogen-deficient but helium-rich superluminous supernova SN 2021bnw which reached a magnitude of -20.7 at maximum luminosity…

astro-ph.HE2025★ 2 cited

Pulsar B1237+25 at 111~MHz: average profile, mode switching, nullings, microstructure

M. V. Popov, T. V. Smirnova

The observations of B1237+25 at a frequency of 111 MHz were analyzed. For the first time in the normal radiation mode a new component in the central region in the average profile w…

astro-ph.HE2025★ 3 cited

Multi-messenger flare in the quasar PKS 0446+11

Y. Y. Kovalev, M. F. Aller, A. K. Erkenov +15

The physical mechanisms driving neutrino and electromagnetic flares in blazars remain poorly understood. We investigate a prominent multi-messenger flare in the quasar PKS 1424+240…

astro-ph.HE2025★ 1 cited

Jet MHD analytical model - framework for radiative transfer

E. E. Nokhrina, I. N. Pashchenko, V. A. Frolova +1

We developed the full magnetohydrodynamical analytical jet model that allows accurate reproducing of a transversal and longitudinal structure for a highly collimated relativistic j…

astro-ph.HE2025★ 3 cited

Dim cores of radio-bright AGN jets: VLBI and Gaia astrometry pinpoint different parsec-scale features

A. V. Popkov, Y. Y. Kovalev, A. V. Plavin +2

Astrometry with the very long baseline radio interferometry (VLBI) allows to determine the position of a point close to the source's brightest compact detail at milliarcsecond scal…

astro-ph.HE2025

On the angular anisotropy of the distribution function of radiating particles in relativistic jets

T. I. Khalilov, V. S. Beskin, V. I. Pariev

The observed power-law spectra of relativistic jets from active galactic nuclei clearly indicate a synchrotron mechanism of radiation by particles that similarly possess a power-la…

astro-ph.HE2025★ 2 cited

Acceleration Potential and Density Profile of Secondary Plasma in the Magnetosphere of Orthogonal Pulsars

A. Yu. Istomin, F. A. Kniazev, V. S. Beskin

A new method for determining the accelerating potential above the polar caps of radio pulsars with an arbitrary inclination angle of the magnetic axis to the rotation axis has been…

astro-ph.HE2025★ 8 cited

Looking into the Jet Cone of the Neutrino-Associated Very High Energy Blazar PKS 1424+240

Y. Y. Kovalev, A. B. Pushkarev, J. L. Gomez +7

The acceleration process of massive particles as well as the production of very high energy (VHE) photons and neutrinos remains a fundamental challenge in astrophysics. We investig…

astro-ph.HE2025★ 2 cited

Search for interpulses in a complete sample of pulsars at a frequency of 111 MHz

M. O. Toropov, S. A. Tyul'bashev, V. S. Beskin

An interpulse search was carried out in a sample of 96 pulsars observed on the Large Phased Array (LPA) radio telescope in the Pushchino Multibeams Pulsar Search (PUMPS). The pulsa…

astro-ph.HE2024★ 2 cited

Sources and Radiations of the Fermi Bubbles

Vladimir A. Dogiel, Chung-Ming Ko

Two enigmatic gamma-ray features in the Galactic central region, known as Fermi Bubbles (FBs), were found from Fermi-LAT data. An energy release (e.g., by tidal disruption events i…

astro-ph.HE2024★ 3 cited

On the possible core shift break in relativistic jets

E. E. Nokhrina

Measurement of a jet geometry transition region is an important instrument of assessing the jet ambient medium properties, plasma bulk motion acceleration, parameters of a black ho…

astro-ph.HE2024★ 15 cited

SN 2023ixf -- an average-energy explosion with circumstellar medium and a precursor

Alexandra Kozyreva, Andrea Caputo, Petr Baklanov +2

Abridged: The fortunate proximity of the SN2023ixf allowed astronomers to follow its evolution from almost the moment of the collapse of the progenitor's core. SN2023ixf can be exp…

astro-ph.HE2024★ 1 cited

Primary and secondary source of energy in the superluminous supernova 2018ibb

Alexandra Kozyreva, Luke Shingles, Petr Baklanov +2

We examine the pair-instability origin of superluminous supernova 2018ibb. As the base model, we use a non-rotating stellar model with an initial mass of 250 Msun at about 1/15 sol…

astro-ph.HE2024★ 1 cited

Spin-down of a pulsar with a yielding crust

Denis Nikolaevich Sob'yanin

In light of the discovery of the long-period radio pulsar PSR J0901-4046, it is interesting to revisit a question about how the magnetized neutron star slows down its rotation. In…

astro-ph.HE2024★ 17 cited

Evidence for a toroidal magnetic field in the core of 3C 84

G. F. Paraschos, L. C. Debbrecht, J. A. Kramer +13

The spatial scales of relativistic radio jets, probed by relativistic magneto-hydrodynamic jet launching simulations (RMHDs) and by most very-long-baseline interferometry (VLBI) ob…

astro-ph.HE2024★ 10 cited

Pushchino multibeams pulsar search. IV. Detection of new pulsars at declinations -9o < δ< +55o

S. A. Tyul'bashev, G. E. Tyul'basheva, M. A. Kitaeva +3

The search for pulsars in monitoring data obtained at the radio telescope Large Phased Array (LPA) at a frequency of 111 MHz was carried out. Daily round-the-clock observations wer…

astro-ph.HE2024

Pushchino multibeams pulsar search -- III. Drift periods of pulsars from summed power spectra method

T. V. Smirnova, S. A. Tyul'bashev, M. A. Kitaeva +1

The drift periods P2 and P3 were searched for using the summed power spectra of 41 pulsars observed at declinations from -9o to +42o. The power spectra of pulses with a given perio…