activity
20122026
most citedThe ASTRO-H X-ray Observatory

106 citations · 117 across the 10 of their papers we have counts for

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astro-ph.HE2026

Nuclear Millimeter Continuum Emission in Radio-Quiet Active Galactic Nuclei: an ALMA Spectral and Variability Study

Sophie M. Venselaar, Claudio Ricci, Yoshiyuki Inoue +8

Unresolved millimeter (mm) emission is observed in radio-quiet (RQ) Active Galactic Nuclei (AGN), but its physical origin remains debated. Self-absorbed synchrotron emission from t…

astro-ph.HE2026

XMM-Newton Resolves Parsec-scale X-ray Jets in the PeVatron Microquasar V4641 Sgr

Naomi Tsuji, Caterina Tresoldi, Kaya Mori +34

The microquasar V4641 Sagittarii (V4641 Sgr) has recently been established as one of the most powerful Galactic PeV cosmic-ray accelerators (PeVatrons) through the detection of deg…

astro-ph.HE2026

Disk truncation triggers relativistic jet launching of a highly accreting supermassive black hole

Hirofumi Noda, Kazuhiro Hada, Hiroto Maruyama +10

Relativistic jets are among the most energetic phenomena in the Universe and influence galaxy evolution through energetic feedback, yet the physical connection between accretion fl…

astro-ph.HE2025★ 1 cited

The first proper motion measurement of the acceleration regions in the large-scale jets of SS 433 powering the W50 nebula

Naomi Tsuji, Yoshiyuki Inoue, Dmitry Khangulyan +10

We report on new Chandra ACIS-I observations of the X-ray knots located in the western and eastern lobes of W50 associated with the parsec-scale jets of the Galactic microquasar SS…

astro-ph.HE2025

X-ray Study on Propagation of Non-thermal Particles in Microquasar SS 433/W 50 Extended Jets

Kazuho Kayama, Takaaki Tanaka, Hiroyuki Uchida +5

SS 433, located at the center of the W 50 radio nebula, is a binary system that ejects jets oriented east-west with precessional motion. X-ray lobes, containing compact "knots" lab…

astro-ph.HE2024★ 4 cited

On the possible contributions of two nearby blazars to the NGC 4151 neutrino hotspot

Anastasiia Omeliukh, Samuel Barnier, Yoshiyuki Inoue

The origin of the high-energy astrophysical neutrinos discovered by IceCube remains unclear, with both blazars and Seyfert galaxies emerging as potential sources. Recently, the Ice…

astro-ph.HE2024★ 3 cited

Multi-epoch X-ray spectral analysis of Centaurus A: revealing new constraints on iron emission line origins

Toshiya Iwata, Atsushi Tanimoto, Hirokazu Odaka +3

We conduct X-ray reverberation mapping and spectral analysis of the radio galaxy Centaurus A to uncover its central structure. We compare the light curve of the hard X-ray continuu…

astro-ph.HE2024★ 2 cited

The possibility of multi-TeV secondary gamma rays from GRB221009A

Oleg Kalashev, Felix Aharonian, Warren Essey +2

The brightest gamma ray burst (GRB) ever observed, GRB221009A, produced a surprisingly large flux of gamma rays with multi-TeV energies, which are expected to be absorbed in intera…

astro-ph.HE2024★ 1 cited

Neutrinos and gamma rays from beta decays in an active galactic nucleus NGC 1068 jet

Koichiro Yasuda, Nobuyuki Sakai, Yoshiyuki Inoue +1

We show that TeV neutrinos and high-energy gamma rays detected from the nearby active galaxy NGC 1068 can simultaneously be explained in a model based on the beta decays of neutron…

astro-ph.HE2024

Upper Limit on the Coronal Cosmic Ray Energy Budget in Seyfert Galaxies

Yoshiyuki Inoue, Shinsuke Takasao, Dmitry Khangulyan

The IceCube collaboration has reported possible detections of high-energy neutrinos from nearby Seyfert galaxies. While central hot coronae are proposed as the primary neutrino pro…