Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Shota Oizumi"'
Autor:
Risako Matsui, Taichi Kato, Hiroyuki Tanaka, Daisaku Nogami, Mahito Sasada, Takashi Ohsugi, Koji S. Kawabata, A. Imada, M. Isogai, Yasushi Fukazawa, Kaori Kubota, Osamu Nagae, Masaru Kino, Shota Oizumi, Toshihiro Omodaka, Shuji Sato, Y. Moritani, T. Uehara, Hisashi Miyamoto, Makoto Uemura, Akira Arai, Hiroyuki Maehara, Takuya Yamashita
Publikováno v:
Publications of the Astronomical Society of Japan. 62:187-199
We report the observation of a new dwarf nova, OT J055717+683226, during its first-ever recorded superoutburst in December 2006. Our observation shows that this object is an SU UMa-type dwarf nova having a very short superhump period of 76.67+/- 0.03
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd7f68cd24f959ad7bcbe3fb2f93f3b6
https://doi.org/10.1093/pasj/62.1.187
https://doi.org/10.1093/pasj/62.1.187
Autor:
Kenshi Yanagisawa, Yoshihiro Arao, Kei Sugiyasu, Tatsuki Yasuda, Shunsuke Tanada, Takeshi Matsuo, Yuuki Moritani, J. Pietz, Hiroyuki Maehara, Taichi Kato, Daisaku Nogami, Miho Suzuki, Hiroyuki Yamamoto, Kie Kodama, Masanao Sumiyoshi, Kazuhiro Nakajima, Shota Oizumi, Akira Imada, Toshihiro Omodaka
We present time-resolved CCD photometry of a dwarf nova NSV 4838 (UMa 8, SDSS J102320.27+440509.8) during the 2005 June and 2007 February outburst. Both light curves showed superhumps with a mean period of 0.0699(1) days for the 2005 outburst and 0.0
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3b454006b07ad95a13144e173d94be4
http://arxiv.org/abs/0902.1013
http://arxiv.org/abs/0902.1013
Autor:
Hiroyuki Yamamoto, Ryoko Ishioka, Kenji Tanabe, Miho Suzuki, Kazuhiro Nakajima, Taichi Kato, Makoto Uemura, Kie Kodama, Ken'ichi Torii, Pavol A. Dubovsky, Shota Oizumi, Kei Sugiyasu, Tatsuki Yasuda, Toshihiro Omodaka, Daisaku Nogami, Koichi Morikawa, Hiroyuki Maehara, Akira Imada, Shunsuke Tanada, Takeshi Matsuo, Kaori Kubota, Yoshihiro Arao
We report on time-resolved CCD photometry of four outbursts of a short-period SU UMa-type dwarf nova, V844 Herculis. We successfully determined the mean superhump periods to be 0.05584(64) days, and 0.055883(3) for the 2002 May superoutburst, and the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d03a8fff94abe50efb69974fff76ff9
Autor:
Katsunori M. Shibata, Seiji Kameno, Miyuki Tsushima, Akiharu Nakagawa, Naoko Matsumoto, Shota Oizumi, Hiroshi Imai, Toshihiro Omodaka, Motonobu Shintani, Tomoharu Kurayama, Makoto Matsui, Yoshihiro Arao, Tatsuki Yasuda
Publikováno v:
Proceedings of the International Astronomical Union. 3:326-327
We have started a VLBI monitoring program for Asymptotic Giant Branch (AGB) stars at 22 and 43 GHz as part of a project of the VLBI Exploration of Radio Astrometry (VERA) for precisely obtaining the period-luminosity (PL) relation of Galactic Mira va
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::14219cc561d1cd992e2b3dbb36bbdc45
https://doi.org/10.1017/s1743921307013257
https://doi.org/10.1017/s1743921307013257