Zobrazeno 1 - 10
of 107
pro vyhledávání: '"R. Ishioka"'
Akademický článek
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Autor:
Katsura Matsumoto, Tansel Ak, Miho Kawabata, Tomohito Ohshima, Hide Akazawa, Ömer Ayyıldız, R. Ishioka, Önder Orakoğlu, Chikako Nakata, Hasan Esenoğlu, Turker Ozkan, Emre Bektöre, Tolga Guver, Linda Schmidtobreick, Metin Altan, Kazunari Masumoto, Makoto Uemura, Antonio Bianchini, Taichi Kato, Takafumi Hori
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 489:1451-1462
The cataclysmic variable SDSS J214354.59+124457.8 (hereafter SDSS J214354) was observed photometrically on sixty one nights between 2012 July 28 and 2019 May 26. The long term variation of this object shows changes between two phases; a dwarf nova ty
Akademický článek
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Autor:
Kirill A. Antonyuk, Taichi Kato, Takafumi Hori, Julia V. Babina, Kem H Cook, Teruaki Enoto, Elena D. Mazaeva, Matthew J. Lehner, Yutaka Maeda, M. Andreev, Kiyoshi Kasai, Tim Axelrod, Nikolai V. Pit, Lewis M. Cook, Wen Ping Chen, Atsushi Miyashita, Alina A. Volnova, J.-H. Wang, Naoto Kojiguchi, Yong-Ik Byun, Typhoon Lee, Megan E. Schwamb, Roger D. Pickard, Tamás Tordai, I. Reva, S. L. Marshall, Enrique de Miguel, Ian Miller, Hiromitsu Takahashi, R. Ishioka, Pavol A. Dubovsky, S. Schmalz, S. K. King, Oksana I. Antonyuk, Katsura Matsumoto, Z. W. Zhang, Yuki Sugiura, Akira Imada, Javier Ruiz, Igor Molotov, Colin Littlefield, Alexei Pozanenko, Federica B. Bianco, Megumi Shidatsu, Aleksei A. Sosnovskij, Nicholas D. James, Yoshihiro Ueda, Charles Alcock, Eiji Yamada, Sergei P. Belan, Makoto Uemura, Keisuke Isogai, Michael Richmond, Seiichiro Kiyota, Dae-Won Kim, William N. Goff, Satoshi Nakahira, William Stein, Shiang-Yu Wang, Mariko Kimura, Elena P. Pavlenko, Ying-Tung Chen, Daisaku Nogami, Aleksei V. Baklanov, C. Y. Wen, R. Inasaridze, Nao Takeda, N. Tungalag
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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arXiv:1607.06195v1.-- et al.
How black holes accrete surrounding matter is a fundamental yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black holes via accretion disks, the state of which depends pri
How black holes accrete surrounding matter is a fundamental yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black holes via accretion disks, the state of which depends pri
Publikováno v:
The Astrophysical Journal. 900:195
Autor:
Katsura Matsumoto, Elena P. Pavlenko, O. V. Vozyakova, Kenzo Kinugasa, Lewis M. Cook, Richard Sabo, Satoshi Honda, R. Ishioka, Sergey Yu. Shugarov, Michael Richmond, Hiroshi Itoh, Taichi Kato, Hiroyuki Maehara, Hikaru Taguchi, Stephen M. Brincat, Mariko Kimura, Raul Michel, Roger D. Pickard, Daisaku Nogami, Nikolai V. Pit, Natalia Katysheva, Kazuhiro Nakajima, Yuki Sugiura, Osamu Hashimoto, Tamás Tordai, Kenji Tanabe, Oksana I. Antonyuk, Geoff Stone, Seiichiro Kiyota, Berto Monard, William N. Goff, Aleksei A. Sosnovskij, Kenta Yamamura, Ian Miller, Shihei Tei, Colin Littlefield, P. Golysheva, Naoto Kojiguchi
Publikováno v:
Publications of the Astronomical Society of Japan. 70
There are several peculiar long-period dwarf-nova like objects, which show rare, low-amplitude outbursts with highly ionized emission lines. 1SWASP J162117$+$441254, BD Pav, and V364 Lib belong to this kind of objects. Some researchers even doubt whe
Autor:
R. Kokumbaeva, R. Ishioka
Publikováno v:
Information Bulletin on Variable Stars.
We present the time series analysis of CCD photometry from ``EAST'' Zeiss-1000 telescope at Tien-Shan Astronomical Observatory (Almaty, Kazakhstan) for GSC 02505-00411. GSC 02505-00411 is a new multi-frequency delta Scuti variable with a primary freq
Autor:
Abigail Holmes, Daniel R. Weisz, Tuan Do, R. Ishioka, Bruno Leibundgut, Wolfgang Kerzendorf, Chuan Jui Li, Kuo-Chuan Pan, T. W. Chen, Paul M. Ricker, You-Hua Chu, Robert A. Gruendl
Publikováno v:
The Astrophysical Journal. 886:99
We have used two methods to search for surviving companions of Type Ia supernova progenitors in three Balmer-dominated supernova remnants in the Large Magellanic Cloud: 0519–69.0, 0505–67.9 (DEM L71), and 0548–70.4. In the first method, we use
Akademický článek
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Publikováno v:
Astrophysics. 54:483-495
Results are presented from photometric studies of the dwarf nova V1108 Her conducted at the primary focus of the 2.6-m G. A. Shajn Telescope at the Crimean Astrophysical Observatory during June-July 2008, 4 years after the 2004 outburst. An orbital p