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 | 日本語 |
発行・発表の年月 | 2022/12/28 |
形態種別 | 学術雑誌 |
標題 | X-Ray Polarization Observations of BL Lacertae |
執筆形態 | 共著 |
掲載誌名 | The Astrophysical Journal Letters |
掲載区分 | 国外 |
出版社・発行元 | American Astronomical Society |
巻・号・頁 | 942(1),L10頁 |
国際共著 | 国際共著 |
著者・共著者 | Riccardo Middei, Ioannis Liodakis, Matteo Perri, Simonetta Puccetti, Elisabetta Cavazzuti, Laura Di Gesu, Steven R. Ehlert, Grzegorz Madejski, Alan P. Marscher, Herman L. Marshall, Fabio Muleri, Michela Negro, Svetlana G. Jorstad, Beatriz Agís-González, Iván Agudo, Giacomo Bonnoli, Maria I. Bernardos, Víctor Casanova, Maya García-Comas, César Husillos, Alessandro Marchini, Alfredo Sota, Pouya M. Kouch, Elina Lindfors, George A. Borman, Evgenia N. Kopatskaya, Elena G. Larionova, Daria A. Morozova |
概要 | Blazars are a class of jet-dominated active galactic nuclei with a typical double-humped spectral energy distribution. It is of common consensus that the synchrotron emission is responsible for the low frequency peak, while the origin of the high frequency hump is still debated. The analysis of X-rays and their polarization can provide a valuable tool to understand the physical mechanisms responsible for the origin of high-energy emission of blazars. We report the first observations of BL Lacertae (BL Lac) performed with the Imaging X-ray Polarimetry Explorer, from which an upper limit to the polarization degree ΠX < 12.6% was found in the 2–8 keV band. |
DOI | 10.3847/2041-8213/aca281 |
ISSN | 20418205 |
NAID | 1360580232390828544 |