Accès ouvert
2026
article
OpenAlex
A. Acharyya, F. Aharonian, F. Ait Benkhali, A. Alkan et autres
The blazar PKS 0903 - 57 has recently been classified as a flat spectrum radio quasar at a redshift of z=0.2621. In March and April 2020, Fermi -LAT and AGILE reported tremendous activity in high-energy γ rays with the flux increasing by …
2026
article
OpenAlex
F. Aharonian, H. Ashkar, M. Backes, R. Batzofin et autres
Context. HESS J0852−463 is a TeV γ-ray source located in the Galactic plane. The region consists of a supernova remnant (SNR, RX J0852.0−4622) with a shell-like morphology, commonly referred to as Vela Junior, and a pulsar named PSR J0855−4644. Pulsars are among …
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2026
article
OpenAlex
A. Acharyya, F. Aharonian, F. Ait Benkhali, A. Alkan et autres
International audience
Accès ouvert
2026
article
OpenAlex
A. Acharyya, F. Aharonian, F. Ait Benkhali, A. Alkan et autres
The blazar PKS 0903-57 has recently been classified as a flat spectrum radio quasar at a redshift of $z=0.2621$. In March and April 2020, Fermi-LAT and AGILE reported tremendous activity in high-energy $γ$ rays with the flux increasing by $\sim$2 orders of …
Accès ouvert
2026
preprint
OpenAlex
A. Acharyya, F. Aharonian, F. Ait Benkhali, A. Alkan et autres
The blazar PKS 0903-57 has recently been classified as a flat spectrum radio quasar at a redshift of $z=0.2621$. In March and April 2020, Fermi-LAT and AGILE reported tremendous activity in high-energy $γ$ rays with the flux increasing by $\sim$2 orders of …
ie, de, fr, Afrique du Sud, gb, rs, pl, Namibie, au, sk, nl, am, at
(code pays fourni par la source)
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2026
article
OpenAlex
F. Aharonian, H. Ashka, M. Backes, R. Batzofin et autres
HESS J0852-463 is a TeV γ-ray source located in the Galactic plane. The region consists of a supernova remnant (SNR, RX J0852.0-4622) with a shell-like morphology, commonly referred to as Vela Junior, and a pulsar denoted PSR J0855-4644. Pulsars are among the …
no
(code pays fourni par la source)
Accès ouvert
2026
preprint
OpenAlex
F. Aharonian, H. Ashkar, M. Backes, R. Batzofin et autres
HESS J0852-463 is a TeV γ-ray source located in the Galactic plane. The region consists of a supernova remnant (SNR, RX J0852.0-4622) with a shell-like morphology, commonly referred to as Vela Junior, and a pulsar denoted PSR J0855-4644. Pulsars are among the …
fr, de, at, pl, Afrique du Sud, au
(code pays fourni par la source)
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2026
article
OpenAlex
(FACT Collaboration), (H.E.S.S. Collaboration), (MAGIC Collaboration), (VERITAS Collaboration) et autres
The search for sources of high-energy astrophysical neutrinos can be significantly advanced through a multimessenger approach, which seeks to detect the γ-rays that accompany neutrinos as they are produced at their sources. Multimessenger observations have so far provided the first evidence for …
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2026
article
OpenAlex
F. Aharonian, H. Ashkar, F. Brun, Q. Remy et autres
Context. HESS J0852−463 is a TeV γ-ray source located in the Galactic plane. The region consists of a supernova remnant (SNR, RX J0852.0−4622) with a shell-like morphology, commonly referred to as Vela Junior, and a pulsar named PSR J0855−4644. Pulsars are among …
Accès ouvert
2023
preprint
OpenAlex
The Cherenkov Telescope Array Consortium, Shotaro Abe, K. Abe, S Abe et autres
Galaxy clusters are expected to be dark matter (DM) reservoirs and storage rooms for the cosmic-ray protons (CRp) that accumulate along the cluster's formation history. Accordingly, they are excellent targets to search for signals of DM annihilation and decay at gamma-ray energies …
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2023
article
OpenAlex
K. Abe, S. Abe, N.Alvarez-Crespo, V. Conforti et autres
Galaxy clusters are expected to be dark matter (DM) reservoirs and storage rooms for the cosmic-ray protons (CRp) that accumulate along the cluster's formation history. Accordingly, they are excellent targets to search for signals of DM annihilation and decay at gamma-ray energies …
fr
(code pays fourni par la source)
Accès ouvert
2022
preprint
OpenAlex
R. Mishra, M. Čemeljić, W. Kluźniak
We investigate accretion onto a central star, with the size, rotation rate, and magnetic dipole of a young stellar object, to study the flow pattern (velocity and density) of the fluid within and outside of the disc. We perform resistive MHD simulations …