Miho Kawabata
Hiroshima University
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Publication
Featured researches published by Miho Kawabata.
The Astrophysical Journal | 2014
Koji S. Kawabata; Hiroshi Akitaya; Masayuki Yamanaka; R. Itoh; Keiichi Maeda; Yuki Moritani; Takahiro Ui; Miho Kawabata; Kensho Mori; Daisaku Nogami; K. Nomoto; Naotaka Suzuki; Katsutoshi Takaki; Masaomi Tanaka; Issei Ueno; Shingo Chiyonobu; Tatsuya Harao; Risako Matsui; Hisashi Miyamoto; Osamu Nagae; Asami Nakashima; Hidehiko Nakaya; Yuma Ohashi; T. Ohsugi; Tomoyuki Komatsu; Kiyoshi Sakimoto; Mahito Sasada; H. Sato; Hiroyuki Tanaka; Takeshi Urano
We presented optical and near-infrared multi-band linear polarimetry of the highly reddened Type Ia SN~2014J appeared in M82. SN~2014J exhibits large polarization at shorter wavelengths, e.g.,
The Astrophysical Journal | 2015
Keiichi Maeda; T. Hattori; D. Milisavljevic; Gaston Folatelli; Maria Rebecca Drout; Hanindyo Kuncarayakti; Raffaella Margutti; Atish Kamble; Alicia M. Soderberg; Masaomi Tanaka; Miho Kawabata; Koji S. Kawabata; Masayuki Yamanaka; K. Nomoto; Ji Hoon Kim; J. D. Simon; Mark M. Phillips; Jerod T. Parrent; Tatsuya Nakaoka; Takashi J. Moriya; Akira Suzuki; Katsutoshi Takaki; Miho N. Ishigaki; Itsuki Sakon; Akito Tajitsu; Masanori Iye
4.8
Publications of the Astronomical Society of Japan | 2014
Taichi Kato; Franz-Josef Hambsch; Hiroyuki Maehara; Gianluca Masi; Francesca Nocentini; Pavol A. Dubovsky; Igor Kudzej; Kazuyoshi Imamura; Minako Ogi; Kenji Tanabe; Hidehiko Akazawa; Thomas Krajci; Ian Miller; Enrique de Miguel; Arne A. Henden; Ryo Noguchi; Takehiro Ishibashi; Rikako Ono; Miho Kawabata; Hiroshi Kobayashi; Daisuke Sakai; Hirochika Nishino; Hisami Furukawa; Kazunari Masumoto; Katsura Matsumoto; Colin Littlefield; Tomohito Ohshima; Chikako Nakata; Satoshi Honda; Kenzo Kinugasa
\% in
Publications of the Astronomical Society of Japan | 2017
Masaomi Tanaka; Yousuke Utsumi; Paolo A. Mazzali; Nozomu Tominaga; Michitoshi Yoshida; Yuichiro Sekiguchi; Kentaro Motohara; Kouji Ohta; Koji S. Kawabata; F. Abe; Kentaro Aoki; Y. Asakura; Stefan Baar; Sudhanshu Barway; I. 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
B
Publications of the Astronomical Society of Japan | 2017
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; Kentaro Motohara; Fumiaki Nakata; Ryou Ohsawa; Kouji Ohta; Hirofumi Okita; Akito Tajitsu; Ichi Tanaka; Tsuyoshi Terai; Naoki Yasuda; F. Abe; Y. Asakura; I. A. Bond; Shota Miyazaki; T. Sumi; P. J. Tristram; Satoshi Honda; R. Itoh
band, and the polarization decreases rapidly at longer wavelengths, with the position angle of the polarization remaining at approximately
Publications of the Astronomical Society of Japan | 2015
Taichi Kato; Franz-Josef Hambsch; Pavol A. Dubovsky; Igor Kudzej; Berto Monard; Ian Miller; Hiroshi Itoh; Seiichiro Kiyota; Kazunari Masumoto; Daiki Fukushima; Hiroki Kinoshita; Kazuki Maeda; Jyunya Mikami; Risa Matsuda; Naoto Kojiguchi; Miho Kawabata; Megumi Takenaka; Katsura Matsumoto; Enrique de Miguel; Yutaka Maeda; Tomohito Ohshima; Keisuke Isogai; Roger D. Pickard; Arne A. Henden; Stella Kafka; Hidehiko Akazawa; Noritoshi Otani; Sakiko Ishibashi; Minako Ogi; Kenji Tanabe
40^{\circ}
Publications of the Astronomical Society of Japan | 2014
Taichi Kato; Pavol A. Dubovsky; Igor Kudzej; Franz-Josef Hambsch; Ian Miller; Tomohito Ohshima; Chikako Nakata; Miho Kawabata; Hirochika Nishino; Kazunari Masumoto; Sahori Mizoguchi; Masayuki Yamanaka; Katsura Matsumoto; Daisuke Sakai; Daiki Fukushima; Minami Matsuura; Genki Bouno; Megumi Takenaka; Shinichi Nakagawa; Ryo Noguchi; Eriko Iino; Roger D. Pickard; Yutaka Maeda; Arne A. Henden; Kiyoshi Kasai; Seiichiro Kiyota; Hidehiko Akazawa; Kazuyoshi Imamura; Enrique de Miguel; Hiroyuki Maehara
over the observed wavelength range. These polarimetric properties suggest that the observed polarization is likely to be caused predominantly by the interstellar dust within M82. Further analysis shows that the polarization peaks at a wavelengths much shorter than those obtained for the Galactic dust. The wavelength dependence of the polarization can be better described by an inverse power law rather than by Serkowski law for Galactic interstellar polarization. These suggests that the nature of the dust in M82 may be different from that in our Galaxy, with polarizing dust grains having a mean radius of
Publications of the Astronomical Society of Japan | 2013
Chikako Nakata; Tomohito Ohshima; Taichi Kato; Daisaku Nogami; Gianluca Masi; Enrique de Miguel; Joseph Ulowetz; Colin Littlefield; William N. Goff; Thomas Krajci; Hiroyuki Maehara; William Stein; Richard Sabo; Ryo Noguchi; Rikako Ono; Miho Kawabata; Hisami Furukawa; Katsura Matsumoto; Takehiro Ishibashi; Pavol A. Dubovsky; Igor Kudzej; Shawn Dvorak; Franz-Josef Hambsch; Roger D. Pickard; Etienne Morelle; Eddy Muyllaert; Stefano Padovan; Arne A. Henden
<0.1\ \mu
Publications of the Astronomical Society of Japan | 2017
Michitoshi Yoshida; Yousuke Utsumi; Nozomu Tominaga; Masaomi Tanaka; Y. Asakura; Kazuya Matsubayashi; Kouji Ohta; F. Abe; Sho Chimasu; Hisanori Furusawa; R. Itoh; Yoichi Itoh; Yuka Kanda; Koji S. Kawabata; Miho Kawabata; Shintaro Koshida; N. Koshimoto; Daisuke Kuroda; Yuki Moritani; Kentaro Motohara; Katsuhiro L. Murata; Takahiro Nagayama; Tatsuya Nakaoka; Fumiaki Nakata; Tsubasa Nishioka; Yoshihiko Saito; Tsuyoshi Terai; P. J. Tristram; Kenshi Yanagisawa; Naoki Yasuda
m.
The Astrophysical Journal | 2016
R. Itoh; Krzysztof Nalewajko; Yasushi Fukazawa; Makoto Uemura; Y. Tanaka; Koji S. Kawabata; G. M. Madejski; F. K. Schinzel; Yuka Kanda; Kensei Shiki; Hiroshi Akitaya; Miho Kawabata; Yuki Moritani; Tatsuya Nakaoka; T. Ohsugi; Mahito Sasada; Katsutoshi Takaki; Koji Takata; Takahiro Ui; Masayuki Yamanaka; Michitoshi Yoshida
We report the late-time evolution of Type IIb Supernova (SN IIb) 2013df. SN 2013df showed a dramatic change in its spectral features at ~1 year after the explosion. Early on it showed typical characteristics shared by SNe IIb/Ib/Ic dominated by metal emission lines, while later on it was dominated by broad and flat-topped Halpha and He I emissions. The late-time spectra are strikingly similar to SN IIb 1993J, which is the only previous example clearly showing the same transition. This late-time evolution is fully explained by a change in the energy input from the
