タナカ シュウタ
TANAKA Shuta
田中 周太 所属 青山学院大学 理工学部 物理科学科 職種 助教 |
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発行・発表の年月 | 2022/08 |
形態種別 | 学術雑誌 |
標題 | Spectral break of energetic pulsar wind nebulae detected with wideband X-ray observations |
執筆形態 | 共同 |
掲載誌名 | Publications of the Astronomical Society of Japan |
掲載区分 | 国外 |
出版社・発行元 | Oxford University Press (OUP) |
巻・号・頁 | 74(5),1186-1197頁 |
著者・共著者 | Aya Bamba, Shinpei Shibata, Shuta J Tanaka, Koji Mori, Hiroyuki Uchida, Yukikatsu Terada, Wataru Ishizaki |
概要 | Pulsar wind nebulae (PWNe) are one of the most energetic galactic sources with bright emissions from radio waves to very high-energy gamma-rays. We perform wideband X-ray spectroscopy of four energetic PWNe, N 157 B, PSR J1813−1749, PSR J1400−6325, and G21.5−0.9, with the Suzaku, Chandra, NuSTAR, and Hitomi observatories. A significant spectral break or cut-off feature is found in the hard X-ray band for all the samples, except for N 157 B. The break energies in the broken power-law fitting are in the range of 4–14 keV, whereas the cut-off energies in the cut-off power-law fitting are at 22 keV or higher. The break or cut-off energy does not show a significant correlation with either the spin-down energy or characteristic age of the hosting pulsars. A possible correlation is found between the photon index change in the broken power-law fitting and the X-ray emitting efficiency of the pulsars, although its significance is not high enough to be conclusive. |
DOI | 10.1093/pasj/psac062 |
ISSN | 00046264 |
NAID | 1360861707123150976 |