言語の選択:
 

メニュー/MENU

大学本部国際商経学部社会情報科学部工学研究科理学研究科環境人間学部看護学部情報科学研究科社会科学研究科緑環境景観マネジメント研究科地域資源マネジメント研究科減災復興政策研究科政策科学研究所高度産業科学技術研究所自然・環境科学研究所地域ケア開発研究所先端医療工学研究所総合教育機構学術総合情報センター地域創造機構産学連携・研究推進機構

研究者業績

研究者リスト >> 本田 敏志
 

本田 敏志

 
アバター
研究者氏名本田 敏志
 
ホンダ サトシ
URL
所属兵庫県立大学
部署自然・環境科学研究所 天文科学センター
職名准教授
学位博士(理学)(総合研究大学院大学)
J-Global ID202001012251638629

研究分野

 
  • 自然科学一般 / 天文学 / 

論文

 
 
Yuta Notsu   Adam F. Kowalski   Hiroyuki Maehara   Kosuke Namekata   Kenji Hamaguchi   Teruaki Enoto   Isaiah I. Tristan   Suzanne L. Hawley   James R. A. Davenport   Satoshi Honda   Kai Ikuta   Shun Inoue   Keiichi Namizaki   Daisaku Nogami   Kazunari Shibata   
The Astrophysical Journal   961(2) 189-189   2024年1月
Abstract

We conducted the time-resolved simultaneous optical spectroscopic and photometric observations of mid-M-dwarf flare stars YZ CMi, EV Lac, and AD Leo. Spectroscopic observations were obtained using Apache Point Observatory 3.5 m and Smal...
 
Kai Ikuta   Kosuke Namekata   Yuta Notsu   Hiroyuki Maehara   Soshi Okamoto   Satoshi Honda   Daisaku Nogami   Kazunari Shibata   
The Astrophysical Journal   948(1) 64-64   2023年5月   [査読有り]
Abstract

Starspots and stellar flares are indicators of stellar magnetic activity. The magnetic energy stored around spots is thought to be the origin of flares, but the connection is not completely understood. To investigate the relation betwee...
 
Shun Inoue   Hiroyuki Maehara   Yuta Notsu   Kosuke Namekata   Satoshi Honda   Keiichi Namizaki   Daisaku Nogami   Kazunari Shibata   
The Astrophysical Journal   948(1) 9-9   2023年4月   [査読有り]
Abstract

Stellar coronal mass ejections (CMEs) have recently received much attention for their impacts on exoplanets and stellar evolution. Detecting prominence eruptions, the initial phase of CMEs, as the blueshifted excess component of Balmer ...
 
Keiichi Namizaki   Kosuke Namekata   Hiroyuki Maehara   Yuta Notsu   Satoshi Honda   Daisaku Nogami   Kazunari Shibata   
The Astrophysical Journal   945(1) 61-61   2023年3月   [査読有り]
<jats:title>Abstract</jats:title>
<jats:p>Active M-type stars are known to often produce superflares on the surface. Radiation from stellar (super)flares is important for exoplanet habitability, but the mechanisms are not well understood. In this...
 
Haining Li   Wako Aoki   Tadafumi Matsuno   Qianfan Xing   Takuma Suda   Nozomu Tominaga   Yuqin Chen   Satoshi Honda   Miho N. Ishigaki   Jianrong Shi   Jingkun Zhao   Gang Zhao   
The Astrophysical Journal   931(2) 147-147   2022年6月   [査読有り]
Abstract

We present homogeneous abundance analysis of over 20 elements for 385 very metal-poor (VMP) stars based on the LAMOST survey and follow-up observations with the Subaru Telescope. It is the largest high-resolution VMP sample (including 3...

MISC

 
 
Kosuke Namekata   Takahito Sakaue   Kyoko Watanabe   Ayumi Asai   Hiroyuki Maehara   Yuta Notsu   Shota Notsu   Satoshi Honda   Takako T. Ishii   Kai Ikuta   Daisaku Nogami   Kazunari Shibata   
Astrophysical Journal   851(2)    2017年12月   
Recently, many superflares on solar-type stars have been discovered as white-light flares (WLFs). The statistical study found a correlation between their energies (E) and durations (τ): τ ∝ E0.39, similar to those of solar hard/soft X-ray flares, ...
 
Yousuke Utsumi   Masaomi Tanaka   Nozomu Tominaga   Michitoshi Yoshida   Sudhanshu Barway   Takahiro Nagayama   Tetsuya Zenko   Kentaro Aoki   Takuya Fujiyoshi   Hisanori Furusawa   Koji S. Kawabata   Shintaro Koshida   Chien-Hsiu Lee   Tomoki Morokuma   Kentaro Motohara   Fumiaki Nakata   Ryou Ohsawa   Kouji Ohta   Hirofumi Okita   Akito Tajitsu   Ichi Tanaka   Tsuyoshi Terai   Naoki Yasuda   Fumio Abe   Yuichiro Asakura   Ian A. Bond   Shota Miyazaki   Takahiro Sumi   Paul J. Tristram   Satoshi Honda   Ryosuke Itoh   Yoichi Itoh   Miho Kawabata   Kumiko Morihana   Hiroki Nagashima   Tatsuya Nakaoka   Tomohito Ohshima   Jun Takahashi   Masaki Takayama   Wako Aoki   Stefan Baar   Mamoru Doi   Francois Finet   Nobuyuki Kanda   Nobuyuki Kawai   Ji Hoon Kim   Daisuke Kuroda   Wei Liu   Kazuya Matsubayashi   Katsuhiro L. Murata   Hiroshi Nagai   Tomoki Saito   Yoshihiko Saito   Shigeyuki Sako   Yuichiro Sekiguchi   Yoichi Tamura   Masayuki Tanaka   Makoto Uemura   Masaki S. Yamaguchi   
Publications of the Astronomical Society of Japan   69(6)    2017年12月   
The first detected gravitational wave from a neutron star merger was
GW170817. In this study, we present J-GEM follow-up observations of SSS17a, an
electromagnetic counterpart of GW170817. SSS17a shows a 2.5-mag decline in the
Tex-band from 1.7 da...
 
Masaomi Tanaka   Yousuke Utsumi   Paolo A. Mazzali   Nozomu Tominaga   Michitoshi Yoshida   Yuichiro Sekiguchi   Tomoki Morokuma   Kentaro Motohara   Kouji Ohta   Koji S. Kawabata   Fumio Abe   Kentaro Aoki   Yuichiro Asakura   Stefan Baar   Sudhanshu Barway   Ian A. Bond   Mamoru Doi   Takuya Fujiyoshi   Hisanori Furusawa   Satoshi Honda   Yoichi Itoh   Miho Kawabata   Nobuyuki Kawai   Ji Hoon Kim   Chien-Hsiu Lee   Shota Miyazaki   Kumiko Morihana   Hiroki Nagashima   Takahiro Nagayama   Tatsuya Nakaoka   Fumiaki Nakata   Ryou Ohsawa   Tomohito Ohshima   Hirofumi Okita   Tomoki Saito   Takahiro Sumi   Akito Tajitsu   Jun Takahashi   Masaki Takayama   Yoichi Tamura   Ichi Tanaka   Tsuyoshi Terai   Paul J. Tristram   Naoki Yasuda   Tetsuya Zenko   
Publications of the Astronomical Society of Japan   69(6)    2017年12月   
Recent detection of gravitational waves from a neutron star (NS) merger event
GW170817 and identification of an electromagnetic counterpart provide a unique
opportunity to study the physical processes in NS mergers. To derive properties
of ejected...
 
Tomoki Morokuma   Masaomi Tanaka   Yasuyuki T. Tanaka   Ryosuke Itoh   Nozomu Tominaga   Poshak Gandhi   Elena Pian   Paolo Mazzali   Kouji Ohta   Emiko Matsumoto   Takumi Shibata   Hinako Akimoto   Hiroshi Akitaya   Gamal B. Ali   Tsutomu Aoki   Mamoru Doi   Nana Ebisuda   Ahmed Essam   Kenta Fujisawa   Hideo Fukushima   Shuhei Goda   Yuya Gouda   Hidekazu Hanayama   Yasuhito Hashiba   Osamu Hashimoto   Kenzo Hayashida   Yuichiro Hiratsuka   Satoshi Honda   Masataka Imai   Kanichiro Inoue   Michiko Ishibashi   Ikuru Iwata   Hideyuki Izumiura   Yuka Kanda   Miho Kawabata   Kenji Kawaguchi   Nobuyuki Kawai   Mitsuru Kokubo   Daisuke Kuroda   Hiroyuki Maehara   Hiroyuki Mito   Kazuma Mitsuda   Ryota Miyagawa   Takeshi Miyaji   Yusuke Miyamoto   Kumiko Morihana   Yuki Moritani   Kana Morokuma-Matsui   Kotone Murakami   Katsuhiro L. Murata   Takahiro Nagayama   Kazuki Nakamura   Tatsuya Nakaoka   Kotaro Niinuma   Takafumi Nishimori   Daisaku Nogami   Yumiko Oasa   Tatsunori Oda   Tomohito Ohshima   Yoshihiko Saito   Shuichiro Sakata   Shigeyuki Sako   Yuki Sarugaku   Satoko Sawada-Satoh   Genta Seino   Kazuo Sorai   Takao Soyano   Francesco Taddia   Jun Takahashi   Yuhei Takagi   Katsutoshi Takaki   Koji Takata   Ken'Ichi Tarusawa   Makoto Uemura   Takahiro Ui   Riku Urago   Kazutoshi Ushioda   Jun-Ichi Watanabe   Makoto Watanabe   Satoshi Yamashita   Kenshi Yanagisawa   Yoshinori Yonekura   Michitoshi Yoshida   
Publications of the Astronomical Society of Japan   69(5)    2017年10月   
We present monitoring campaign observations at optical and near-infrared (NIR) wavelengths for a radio-loud active galactic nucleus (AGN) at z = 0.840, SDSS J110006.07+442144.3 (hereafter, J1100+4421), which was identified during a flare phase in ...
 
Tadafumi Matsuno   Wako Aoki   Timothy C. Beers   Young Sun Lee   Satoshi Honda   
Astronomical Journal   154(2)    2017年8月   
We present elemental abundances for eight unevolved extremely metal-poor (EMP) stars with Teff 5500 K, among which seven have [Fe H] -3.5. The sample is selected from the Sloan Digital Sky Survey/Sloan Extension for Galactic Understanding and Expl...

共同研究・競争的資金等の研究課題

 
 
大質量星連星を手がかりとする初代星と重力波起源天体の探査
日本学術振興会: 科学研究費助成事業 基盤研究(C)
須田 拓馬 本田 敏志 斎藤 貴之 森谷 友由希 茂山 俊和 
研究期間: 2022年4月 - 2025年3月
 
明るい金属欠乏星の全北天域探査による初代星元素合成と初期銀河系形成の解明
日本学術振興会: 科学研究費助成事業 基盤研究(A)
青木 和光 冨永 望 諸隈 智貴 本田 敏志 石垣 美歩 平居 悠 野本 憲一 須田 拓馬 
研究期間: 2021年4月 - 2025年3月
 
恒星スーパーフレア解明のための太陽フレアのThe-Sun-as-a-star研究
日本学術振興会: 科学研究費助成事業 基盤研究(B)
柴田 一成 野上 大作 本田 敏志 前原 裕之 浅井 歩 一本 潔 
研究期間: 2021年4月 - 2024年3月
 
太陽白色光フレアの解析に基づく、スーパーフレア星の磁気活動機構の解明
日本学術振興会: 科学研究費助成事業 基盤研究(B)
柴田 一成 野上 大作 本田 敏志 前原 裕之 浅井 歩 一本 潔 磯部 洋明 
研究期間: 2016年4月 - 2019年3月
 
スーパーフレア星の化学組成から探る元素合成の研究
日本学術振興会: 科学研究費助成事業 基盤研究(C)
本田 敏志 
研究期間: 2014年4月 - 2018年3月