Multi-wavelength Photometric and Polarimetric Observations of the Outburst of 3C 454.3 in Dec. 2009
Publications of the Astronomical Society of Japan 64 巻 3 号
58-1-58-8 頁
2012-06-25 発行
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| ファイル情報(添付) | |
| タイトル ( eng ) |
Multi-wavelength Photometric and Polarimetric Observations of the Outburst of 3C 454.3 in Dec. 2009
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| 作成者 |
Itoh Ryosuke
Sakon Itsuki
Fujisawa Kenta
Kadota Akiko
Yasuda Hajimu
Sato Shuji
Kino Masaru
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| 収録物名 |
Publications of the Astronomical Society of Japan
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| 巻 | 64 |
| 号 | 3 |
| 開始ページ | 58-1 |
| 終了ページ | 58-8 |
| 抄録 |
In December 2009, the bright blazar, 3C 454.3 exhibited a strong outburst in the optical, X-ray and gamma-ray regions. We performed photometric and polarimetric monitoring of this outburst in the optical and near-infrared bands with TRISPEC and HOWPol attached to the Kanata telescope. We also observed this outburst in the infrared band with AKARI, and the radio band with the 32-m radio telescope of Yamaguchi University. The object was in an active state from JD 2455055 to 2455159. It was 1.3 mag brighter than its quiescent state before JD 2455055 in the optical band. After the end of the active state in JD 2455159, a prominent outburst was observed in all wavelengths. The outburst continued for two months. Our optical and near-infrared polarimetric observations revealed that the position angle of the polarization (PA) apparently rotated clockwise by 240 degrees within 11 d in the active state (JD 2455063—2455074), and after this rotation, PA remained almost constant during our monitoring. In the outburst state, PA smoothly rotated counterclockwise by 350 degrees within 35 d (JD 2455157—2455192). Thus, we detected two distinct rotation events of polarization vector in opposite directions. We discuss these two events compared with the past rotation events observed in 2005, 2007 and 2008.
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| 著者キーワード |
BL Lacertae Objects: individual: 3C 454.3 — polarization — infrared: general
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| 内容記述 |
This work was partly supported by a Grand-in-Aid from the Ministry of Education, Culture, Sports, Science, and Technology of Japan (22540252,). This research has made use of data from the University of Michigan Radio Astronomy Observatory which has been supported by the University of Michigan and by a series of grants from the National Science Foundation, most recently AST-0607523. The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. M. Sasada and M. Yamanaka have been supported by the JSPS Research Fellowship for Young Scientists.
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| NDC分類 |
天文学・宇宙科学 [ 440 ]
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| 言語 |
英語
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| 資源タイプ | 学術雑誌論文 |
| 出版者 |
Astronomical Society of Japan
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| 発行日 | 2012-06-25 |
| 権利情報 |
Copyright (c) 2012 The Astronomical Society of Japan
This is not the published version. Please cite only the published version. この論文は出版社版でありません。引用の際には出版社版をご確認ご利用ください。
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| 出版タイプ | Author’s Original（十分な品質であるとして、著者から正式な査読に提出される版） |
| アクセス権 | オープンアクセス |
| 収録物識別子 |
[ISSN] 0004-6264
[NCID] AA1082896X
[DOI] 10.1093/pasj/64.3.58
[DOI] https://doi.org/10.1093/pasj/64.3.58
[arXiv] arXiv:1112.4583
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