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A fundamental plane in X-ray binary activity of external galaxies
DOI: 10.1093/pasj/psab077 Bibcode: 2021PASJ...73.1315I

Ueda, Yoshihiro; Inoue, Yoshiyuki; Yabe, Kiyoto

We construct a new catalog of extragalactic X-ray binaries (XRBs) by matching the latest Chandra source catalog with local galaxy catalogs. Our XRB catalog contains 4430 XRBs hosted by 237 galaxies within ~130 Mpc. As XRBs dominate the X-ray activity in galaxies, the catalog enables us to study the correlations between the total X-ray luminosity o…

2021 Publications of the Astronomical Society of Japan
XMM-Newton 7
A study of the accretion mechanisms of the high-mass X-ray binary IGR J00370+6122
DOI: 10.1093/pasj/psab083 Bibcode: 2021PASJ...73.1389U

Fukazawa, Yasushi; Makishima, Kazuo; Takahashi, Hiromitsu +1 more

IGR J00370+6122 is a high-mass X-ray binary with a B1 Ib primary star and a companion suggested to be a neutron star because of the detection of a 346 s pulsation in a one-off 4 ks observation. To better understand the nature of the compact companion, the present work performs timing and spectral studies of the X-ray data of this object, taken wit…

2021 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 5
Suzaku observations of Jovian diffuse hard X-ray emission
DOI: 10.1093/pasj/psab053 Bibcode: 2021PASJ...73..894N

Miyoshi, Yoshizumi; Ezoe, Yuichiro; Ishikawa, Kumi +6 more

We report on results of systematic analyses of the entire three X-ray data sets of Jupiter taken by Suzaku in 2006, 2012, and 2014. Jovian diffuse hard X-ray emission was discovered by Suzaku in 2006 when the solar activity went toward its minimum. The diffuse emission was spatially consistent with the Jovian inner magnetosphere and was spectrally…

2021 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 2
Signatures of large-scale cold fronts in the optically-selected merging cluster HSC J085024+001536
DOI: 10.1093/pasj/psab022 Bibcode: 2021PASJ...73..584T

Oguri, Masamune; Fujimoto, Ryuichi; Okabe, Nobuhiro +5 more

We represent a joint X-ray, weak-lensing, and optical analysis of the optically-selected merging cluster, HSC J085024+001536, from the Subaru HSC-SSP survey. Both the member galaxy density and the weak-lensing mass map show that the cluster is composed of south-east and north-west components. The two-dimensional weak-lensing analysis shows that th…

2021 Publications of the Astronomical Society of Japan
XMM-Newton 1