アキタヤ ヒロシ
秋田谷 洋 所属 千葉工業大学 天文学研究センター 天文学研究センター 職種 上席研究員 |
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言語種別 | 英語 |
発行・発表の年月 | 2016 |
形態種別 | 国際会議プロシーディングス |
標題 | Photometric and Polarimetric Observations of Be/X-Ray and Be/Gamma-Ray Binaries |
執筆形態 | 共著 |
掲載誌名 | BRIGHT EMISSARIES: BE STARS AS MESSENGERS OF STAR-DISK PHYSICS |
掲載区分 | 国外 |
出版社・発行元 | ASTRONOMICAL SOC PACIFIC |
巻・号・頁 | 506,pp.295-298 |
著者・共著者 | Y. Moritani,H. Akitaya,N. Ebisuda,R. Itoh,Y. Kanda,M. Kawabata,K. Kawaguchi,K. Mori,T. Nakaoka,Y. Ohashi,K. Takaki,I. Ueno,T. Ui,T. Urano,M. Yoshida |
概要 | Be/X-ray and Be/gamma-ray binaries are systems comprised of a Be star and a compact object. In these systems, the Be disk plays an important role in their high-energy activities through the interaction with the compact object. Because of highly eccentric orbits, the interaction depends on the orbital phase in Be/X and Be/gamma-ray binaries. Such interaction affects the Be disk structure, causing photometric and polarimetric variabilities. In order to search for photometric and polatimetric variability in Be/X-ray and Be/gamma-ray binaries, we have monitored several systems with the polarimeter attached to Hiroshima 1.5m Kanata telescope, Japan. Our two-year monitor finds that some programmed systems show photometric variations and a few systems show polatimatric variabilities. |