H
Haruka Sakemi
Researcher at Kyushu University
Publications - 10
Citations - 51
Haruka Sakemi is an academic researcher from Kyushu University. The author has contributed to research in topics: Galaxy & Faraday cage. The author has an hindex of 3, co-authored 8 publications receiving 34 citations.
Papers
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Journal ArticleDOI
Magnetic field analysis of the bow and terminal shock of the SS 433 jet
Haruka Sakemi,Mami Machida,Takuya Akahori,Hiroyuki Nakanishi,Hiroki Akamatsu,Kohei Kurahara,Jamie Farnes +6 more
TL;DR: In this article, a polarization analysis of the eastern region of W50, observed with the Australia Telescope Compact Array (ATCA) at 1.4 - 3.0 GHz, was performed and it was shown that the orientation of the intrinsic magnetic field vectors are aligned along the total intensity structures.
Journal ArticleDOI
Magnetic Field Analysis of the Bow and Terminal Shock of the SS433 Jet
Haruka Sakemi,Mami Machida,Takuya Akahori,Hiroyuki Nakanishi,Hiroki Akamatsu,Kohei Kurahara,Jamie Farnes +6 more
TL;DR: In this paper, a polarization analysis of the eastern region of W50, observed with the Australia Telescope Compact Array (ATCA) at 1.4 - 3.0 GHz, was performed and it was shown that the orientation of the intrinsic magnetic field vectors are aligned along the total intensity structures.
Journal ArticleDOI
Jets from MRC 0600-399 bent by magnetic fields in the cluster Abell 3376.
James O. Chibueze,James O. Chibueze,Haruka Sakemi,Takumi Ohmura,Takumi Ohmura,Mami Machida,Hiroki Akamatsu,Takuya Akahori,Hiroyuki Nakanishi,Viral Parekh,Ruby van Rooyen,Tsutomu T. Takeuchi +11 more
TL;DR: In this paper, radio observations of the second-brightest galaxy in the merging galaxy cluster Abell 3376 (redshift 0.0461) were used to detect the double-scythe structures.
Journal ArticleDOI
Faraday tomography of the SS433 jet termination region
Haruka Sakemi,Mami Machida,Takumi Ohmura,Shinsuke Ideguchi,Yoshimitsu Miyashita,Keitaro Takahashi,Takuya Akahori,Hiroki Akamatsu,Hiroyuki Nakanishi,Kohei Kurahara,Jamie Farnes +10 more
TL;DR: In this article, the authors apply QU-fitting to data from the Australia Telescope Compact Array (ATCA) at 1.3-3.0 GHz to identify multiple polarized sources along the line of sight.
Journal ArticleDOI
Energy estimation of high energy particles associated with the SS433/W50 system through radio observation at 1.4 GHz
TL;DR: The radio nebula W50 is a unique object interacting with the jets of the microquasar SS433 as discussed by the authors, which is a good target for investigating the energy of cosmic-ray particles accelerated by galactic jets.