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大学・研究所にある論文を検索できる 「Discovery of Year-scale Time Variability from Thermal X-Ray Emission in Tycho’s Supernova Remnant」の論文概要。リケラボ論文検索は、全国の大学リポジトリにある学位論文・教授論文を一括検索できる論文検索サービスです。
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Discovery of Year-scale Time Variability from Thermal X-Ray Emission in Tycho’s Supernova Remnant

Matsuda, Masamune Uchida, Hiroyuki Tanaka, Takaaki Yamaguchi, Hiroya Tsuru, Takeshi Go 京都大学 DOI:10.3847/1538-4357/ac94cf

2022.12.01

概要

Mechanisms of particle heating are crucial to understanding the shock physics in supernova remnants (SNRs). However, there has been little information on time variabilities of thermalized particles so far. Here, we present a discovery of a gradually brightening thermal X-ray emission found in the Chandra data of Tycho's SNR obtained during 2000–2015. The emission exhibits a knot-like feature (Knot1) with a diameter of ≃0.04 pc located in the northwestern limb, where we also find localized Hα filaments in an optical image taken with the Hubble Space Telescope in 2008. The model with the solar abundance reproduces the spectra of Knot1, suggesting that Knot1 originates from the interstellar medium; this is the first detection of thermal X-ray emission from swept-up gas found in Tycho's SNR. Our spectral analysis indicates that the electron temperature of Knot1 has increased from ∼0.30 to ∼0.69 keV within the period between 2000 and 2015. These results lead us to ascribe the time-variable emission to a small dense clump recently heated by the forward shock at the location of Knot1. The electron-to-proton temperature ratio immediately downstream of the shock (β₀ ≡ Te/Tp) is constrained to be me/mp ≤ β₀ ≤ 0.15 to reproduce the data, indicating the collisionless electron heating with efficiency is consistent with previous Hα observations of Tycho and other SNRs with high shock velocities.

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