activity
20182022
most citedXMM-Newton view of the shock heating in an early merging cluster, CIZA J1358.94750

8 citations · 22 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA20228 cited

XMM-Newton view of the shock heating in an early merging cluster, CIZA J1358.94750

Y. Omiya, K. Nakazawa, K. Matsushita +10

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 o…

astro-ph.GA20227 cited

Physical properties of the molecular cloud, N4, in SS433; Evidence for an interaction of molecular cloud with the jet from SS433

Hiroaki Yamamoto, Ryuji Okamoto, Yasuhiro Murata +3

We conducted observations and analyses of the molecular cloud, N4, which is located at ~40 pc from SS433 and the same line of sight as that of the radio shell, in 12CO(J=1-0), 12CO…

astro-ph.GA20201 cited

Large-scale magnetic field structure of NGC 3627 based on magnetic vector map

Kohei Kurahara, Hiroyuki Nakanishi, Yuki Kudoh

We analyzed the data of Stokes , , and in C- and X-bands and investigated the large-scale magnetic field structure of NGC 3627. The polarization intensity and angle in ea…

astro-ph.GA2019

Outer rotation curve of the Galaxy with VERA IV: Astrometry of IRAS 01123+6430 and the possibility of cloud-cloud collision

Nagito Koide, Hiroyuki Nakanishi, Nobuyuki Sakai +13

As part our investigation into the Galactic rotation curve, we carried out Very Long Baseline Interferometry (VLBI) observations towards the star-forming region IRAS 01123+6430 usi…

astro-ph.GA20194 cited

Magnetic Field Vector Structure of NGC6946

Kohei Kurahara, Hiroyuki Nakanishi

We studied large-scale magnetic field reversals of a galaxy based on a magnetic vector map of NGC6946. The magnetic vector map was constructed based on the polarization maps in the…

astro-ph.GA20192 cited

Magnetic field vector maps of nearby spiral galaxies

Hiroyuki Nakanishi, Kohei Kurahara, Kenta Anraku

We present a method for determining directions of magnetic field vectors in a spiral galaxy using two synchrotron polarization maps, an optical image, and a velocity field. The ori…