Literature DB >> 26738586

Astrophysics: Why black holes pulse brightly.

Poshak Gandhi1.   

Abstract

Year:  2016        PMID: 26738586     DOI: 10.1038/529028a

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


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  2 in total

1.  Repetitive patterns in rapid optical variations in the nearby black-hole binary V404 Cygni.

Authors:  Mariko Kimura; Keisuke Isogai; Taichi Kato; Yoshihiro Ueda; Satoshi Nakahira; Megumi Shidatsu; Teruaki Enoto; Takafumi Hori; Daisaku Nogami; Colin Littlefield; Ryoko Ishioka; Ying-Tung Chen; Sun-Kun King; Chih-Yi Wen; Shiang-Yu Wang; Matthew J Lehner; Megan E Schwamb; Jen-Hung Wang; Zhi-Wei Zhang; Charles Alcock; Tim Axelrod; Federica B Bianco; Yong-Ik Byun; Wen-Ping Chen; Kem H Cook; Dae-Won Kim; Typhoon Lee; Stuart L Marshall; Elena P Pavlenko; Oksana I Antonyuk; Kirill A Antonyuk; Nikolai V Pit; Aleksei A Sosnovskij; Julia V Babina; Aleksei V Baklanov; Alexei S Pozanenko; Elena D Mazaeva; Sergei E Schmalz; Inna V Reva; Sergei P Belan; Raguli Ya Inasaridze; Namkhai Tungalag; Alina A Volnova; Igor E Molotov; Enrique de Miguel; Kiyoshi Kasai; William L Stein; Pavol A Dubovsky; Seiichiro Kiyota; Ian Miller; Michael Richmond; William Goff; Maksim V Andreev; Hiromitsu Takahashi; Naoto Kojiguchi; Yuki Sugiura; Nao Takeda; Eiji Yamada; Katsura Matsumoto; Nick James; Roger D Pickard; Tamás Tordai; Yutaka Maeda; Javier Ruiz; Atsushi Miyashita; Lewis M Cook; Akira Imada; Makoto Uemura
Journal:  Nature       Date:  2016-01-07       Impact factor: 49.962

2.  Cosmic X-ray Sources.

Authors:  S Bowyer; E T Byram; T A Chubb; H Friedman
Journal:  Science       Date:  1965-01-22       Impact factor: 47.728

  2 in total

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