Search Publications

AGN number fraction in galaxy groups and clusters at z < 1.4 from the Subaru Hyper Suprime-Cam survey
DOI: 10.1093/pasj/psad066 Bibcode: 2023PASJ...75.1246H

Goto, Tomotsugu; Imanishi, Masatoshi; Schramm, Malte +20 more

One of the key questions on active galactic nuclei (AGN) in galaxy clusters is how AGN could affect the formation and evolution of member galaxies and galaxy clusters in the history of the Universe. To address this issue, we investigate the dependence of AGN number fraction (fAGN) on cluster redshift (zcl) and distance from t…

2023 Publications of the Astronomical Society of Japan
XMM-Newton 13
MeerKAT's view of double radio relic galaxy cluster Abell 3376
DOI: 10.1093/pasj/psac009 Bibcode: 2023PASJ...75S..97C

Nakanishi, Hiroyuki; Akamatsu, Hiroki; Takeuchi, Tsutomu T. +10 more

We present the initial results of our MeerKAT L-band observations of Abell 3376. We achieved higher (5″) angular resolution and better (~4 µ Jy beam-1) sensitivity compared to the previous observations. Our achieved sensitivity is only a factor of 2 larger than the thermal noise of MeerKAT. Astrometric and flux comparison of discr…

2023 Publications of the Astronomical Society of Japan
XMM-Newton 12
X-ray and optical spectroscopic study of a γ Cassiopeiae analog source π Aquarii
DOI: 10.1093/pasj/psac099 Bibcode: 2023PASJ...75..177T

Tsujimoto, Masahiro; Hayashi, Takayuki; Morihana, Kumiko +1 more

γ Cas analog sources are a subset of Be stars that emit intense and hard X-ray emission. Two competing ideas for their X-ray production mechanism are (a) the magnetic activities of the Be star and its disk and (b) the accretion from the Be star to an unidentified compact object. Among such sources, π Aqr plays a pivotal role as it is one of the on…

2023 Publications of the Astronomical Society of Japan
Gaia XMM-Newton 8
XMM-Newton view of the shock heating in an early merging cluster, CIZA J1358.9-4750
DOI: 10.1093/pasj/psac087 Bibcode: 2023PASJ...75...37O

Sato, Kosuke; Nakazawa, Kazuhiro; Gu, Liyi +10 more

CIZA J1358.9-4750 is a nearby galaxy cluster in the early phase of a major merger. The two-dimensional temperature map using XMM-Newton EPIC-PN observation confirms the existence of a high-temperature region, which we call the "hot region," in the "bridge region" connecting the two clusters. The ~500 kpc wide region between the south-east and nort…

2023 Publications of the Astronomical Society of Japan
XMM-Newton 5
On the influence of shock-cloud interactions on the nonthermal X-ray emission from the supernova remnant RCW 86
DOI: 10.1093/pasj/psad075 Bibcode: 2023PASJ...75.1344B

Vink, Jacco; Bamba, Aya; Sano, Hidetoshi +1 more

The effect of the surrounding environment of supernova remnant shocks on nonthermal X-rays from accelerated electrons, with or without interacting dense material, is an open issue. We conduct spatially resolved X-ray spectroscopy of the shock-cloud interacting region of RCW 86 with XMM-Newton. It is found that bright soft X-ray filaments surround …

2023 Publications of the Astronomical Society of Japan
XMM-Newton 3