Showing 2022 · astro-ph.HEShow all

90 papers · 2 filters

astro-ph.HE2022★ 7 cited

Impact of a binary black hole on its outer circumbinary disc

Raphaël Mignon-Risse, Peggy Varniere, Fabien Casse

Accreting supermassive binary black holes (SMBBHs) are potential targets for multi-messenger astronomy as they emit gravitational waves (GW) while their environment emits electroma…

astro-ph.HE2022★ 1 cited

Interaction of a high-mass X-ray binary with the interstellar medium through stellar wind. The case of GX 301-2

J. Marchioro, S. Chaty, A. Coleiro +2

GX 301-2 is a high-mass X-ray binary (HMXB) with strong stellar outflows. The evolution of these binaries can be closely related with the interstellar environment due to strong win…

astro-ph.HE2022★ 105 cited

The MeerKAT Pulsar Timing Array: First Data Release

Matthew T. Miles, Ryan M. Shannon, Matthew Bailes +15

We present the first 2.5 years of data from the MeerKAT Pulsar Timing Array (MPTA), part of MeerTime, a MeerKAT Large Survey Project. The MPTA aims to precisely measure pulse arriv…

astro-ph.HE2022★ 6 cited

Caustic-like Structures in UHECR Flux after Propagation in Turbulent Intergalactic Magnetic Fields

K. Dolgikh, A. Korochkin, G. Rubtsov +2

UHECR propagation in a turbulent intergalactic magnetic field in the small-angle scattering regime is well understood for propagation distances much larger than the field coherence…

astro-ph.HE2022★ 58 cited

Hint for a TeV neutrino emission from the Galactic Ridge with ANTARES

A. Albert, S. Alves, M. André +151

Interactions of cosmic ray protons, atomic nuclei, and electrons in the interstellar medium in the inner part of the Milky Way produce a -ray flux from the Galactic Ridge. If th…

astro-ph.HE2022★ 12 cited

Standing Accretion Shock Instability in the Collapse of a Rotating Stellar Core

Laurie Walk, Thierry Foglizzo, Irene Tamborra

Hydrodynamical instabilities, such as the standing accretion-shock instability (SASI), play an essential role in the dynamics of core-collapse supernovae, with observable imprints…

astro-ph.HE2022★ 13 cited

Precession of magnetars: dynamical evolutions and modulations on polarized electromagnetic waves

Yong Gao, Lijing Shao, Gregory Desvignes +3

Magnetars are conjectured to be highly magnetized neutron stars (NSs). Strong internal magnetic field and elasticity in the crust may deform the stars and lead to free precession.…

astro-ph.HE2022★ 8 cited

On the evolution of the particle distribution and the cascade in a moving, expanding emission region in blazar jets

Michael Zacharias

There is a large variety in the models explaining blazar flares. Here, we study the flare profile induced by a moving and expanding blob with special emphasize on the gamma-gamma p…

astro-ph.HE2022★ 7 cited

MeV-GeV Gamma-ray Emission from SNR G327.1-1.1 Discovered by the Fermi-LAT

Jordan Eagle, Daniel Castro, Tea Temim +5

We report the discovery of MeV-GeV gamma-ray emission by the Fermi-LAT positionally coincident with the TeV pulsar wind nebula (PWN) HESS~J1554-550 within the host supernova remnan…

astro-ph.HE2022★ 13 cited

Optical Spectroscopy of Blazars for the Cherenkov Telescope Array -- II

E. Kasai, P. Goldoni, S. Pita +11

Active galactic nuclei (AGNs) make up about 35 per cent of the more than 250 sources detected in very-high-energy (VHE) gamma rays to date with Imaging Atmospheric Cherenkov Telesc…

astro-ph.HE2022★ 22 cited

Blazars at Very High Energies: Emission Modelling

Hélène Sol, Andreas Zech

Blazars are very broadband cosmic sources with spectra spanning over twenty orders of magnitude in frequency, down to the 100 MHz regime in the radio range, up to VHE at several te…

astro-ph.HE2022★ 29 cited

Quality over Quantity: Optimizing pulsar timing array analysis for stochastic and continuous gravitational wave signals

Lorenzo Speri, Nataliya K. Porayko, Mikel Falxa +4

The search for gravitational waves using Pulsar Timing Arrays (PTAs) is a computationally expensive complex analysis that involves source-specific noise studies. As more pulsars ar…

astro-ph.HE2022★ 12 cited

Evolution of the afterglow optical spectral shape of GRB 201015A in the first hour: evidence for dust destruction

Toktarkhan Komesh, Bruce Grossan, Zhanat Maksut +3

Instruments such as the ROTSE, TORTORA, Pi of the Sky, MASTER-net, and others have recorded single-band optical flux measurements of gamma-ray bursts starting as early as $\thicksi…

astro-ph.HE2022★ 66 cited

Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Abdul Halim, P. Abreu +365

In this work we present the interpretation of the energy spectrum and mass composition data as measured by the Pierre Auger Collaboration above eV. We use an ast…

astro-ph.HE2022★ 1 cited

Classification of 3 accreting binaries with VLT/X-Shooter spectra

Tristan Bouchet, Sylvain Chaty, Francis Fortin +1

Since its launch, the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) satellite has discovered hundreds of X-ray sources, many of which lack proper classification. This…

astro-ph.HE2022★ 11 cited

A NuSTAR view of SS433: Precessional evolution of the jet-disk system

Federico A. Fogantini, Federico García, Jorge A. Combi +3

SS433 is a Galactic microquasar with powerful outflows (double jet, accretion disk and winds) with well known orbital, precessional and nutational period. In this work we character…

astro-ph.HE2022★ 90 cited

A lower bound on intergalactic magnetic fields from time variability of 1ES 0229+200 from MAGIC and Fermi/LAT observations

MAGIC Collaboration, V. A. Acciari, I. Agudo +206

Extended and delayed emission around distant TeV sources induced by the effects of propagation of gamma rays through the intergalactic medium can be used for the measurement of the…

astro-ph.HE2022

Internal Heating in Magnetars: Role of Electron Captures

Nicolas Chamel, Anthea Francesca Fantina, Lami Suleiman +2

The role of electron captures by nuclei in the shallow heating of magnetars is further investigated using both nuclear measurements and the theoretical atomic mass table HFB-27. St…

astro-ph.HE2022★ 129 cited

The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope -- Data Release 3

LAT collaboration, Marco Ajello, Luca Baldini +100

An incremental version of the fourth catalog of active galactic nuclei (AGNs) detected by the Fermi-Large Area Telescope is presented. This version (4LAC-DR3) derives from the thir…

astro-ph.HE2022★ 12 cited

Gamma-ray observations of MAXI J1820+070 during the 2018 outburst

H. Abe, S. Abe, V. A. Acciari +439

MAXI J1820+070 is a low-mass X-ray binary with a black hole as a compact object. This binary underwent an exceptionally bright X-ray outburst from March to October 2018, showing ev…

astro-ph.HE2022★ 5 cited

A Black-Hole Excision Scheme for General Relativistic Core-Collapse Supernova Simulations

B. Sykes, B. Mueller, I. Cordero-Carrión +2

Fallback supernovae and the collapsar scenario for long-gamma ray burst and hypernovae have received considerable interest as pathways to black-hole formation and extreme transient…

astro-ph.HE2022★ 39 cited

Three-dimensional core-collapse supernovae with complex magnetic structures: II. Rotational instabilities and multi-messenger signatures

Matteo Bugli, Jérôme Guilet, Thierry Foglizzo +1

The gravitational collapse of rapidly rotating massive stars can lead to the onset of the low instability within the central proto-neutron star (PNS), which leaves strong…

astro-ph.HE2022★ 32 cited

Multi-messenger characterization of Mrk 501 during historically low X-ray and -ray activity

MAGIC collaboration, H. Abe, S. Abe +322

We study the broadband emission of Mrk 501 using multi-wavelength observations from 2017 to 2020 performed with a multitude of instruments, involving, among others, MAGIC, Fermi-LA…

astro-ph.HE2022★ 25 cited

High-energy neutrino-induced cascade from the direction of the flaring radio blazar TXS 0506+056 observed by Baikal-GVD in 2021

GVD Collaboration, A. K. Erkenov, N. A. Kosogorov +8

The existence of high-energy astrophysical neutrinos has been unambiguously demonstrated, but their sources remain elusive. IceCube reported an association of a 290-TeV neutrino wi…