Suzaku Observation of the South-East Limb of the Cygnus Loop

机译：朱雀对天鹅座环东南肢的观察

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We observed the south-east (SE) limb (P26, P27, and P28) of the Cygnus Loop supernova remnant (SNR) with Suzaku. The X-ray morphologies of P26 and P28 show concaved structures relative to the other shell regions of the Loop. Levenson et al. (2005) insisted that the concave seen in P26 is due to the interaction of the supernova blast wave with a large scale interstellar cloud from their Chandra observation. We perform spatially resolved spectroscopy for the Suzaku data. Applying a single temperature NEI model, we generate maps of the electron temperature, the ionization time scale, the emission measure, and metal abundances. Based on the maps, we propose that the blast wave is hitting interstellar clouds in P28 as well as P26, while the blast wave is propagating into a relatively uniform ambient medium in P26.

机译：我们观察到了朱雀与天鹅环超新星遗迹（SNR）的东南（SE）肢体（P26，P27和P28）。 P26和P28的X射线形态相对于Loop的其他外壳区域显示出凹入结构。莱文森等。（2005年）坚持认为，在P26中看到的凹面是由于超新星爆炸波与Chandra观测中大规模星际云的相互作用所致。我们对朱雀数据进行空间分辨光谱分析。应用单温度NEI模型，我们生成电子温度，电离时间尺度，发射度量和金属丰度的图。根据这些图，我们建议爆炸波撞击P28和P26中的星际云，而爆炸波传播到P26中相对均匀的环境介质中。

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来源
《The energetic cosmos : from Suzaku to ASTRO-H》|2009年|p.120-121|共2页
会议地点 Hokkaido(JP)
作者
Hiroko Kosugi; Hiroshi Tsunemi; Hiroyuki Uchida; Masashi Kimura; Satoru Katsuda;
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作者单位

Department of Earth and Space Science, Graduate School of Science, Osaka University,1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan;

Department of Earth and Space Science, Graduate School of Science, Osaka University,1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan;

Department of Earth and Space Science, Graduate School of Science, Osaka University,1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan;

Department of Earth and Space Science, Graduate School of Science, Osaka University,1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan;

Code 662, NASA Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.;

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原文格式 PDF
正文语种 eng
中图分类恒星天文学、星系天文学、宇宙学;
关键词
ISM; abundances — ISM; individual (Cygnus Loop) — ISM; supernova remnants —X-rays; ISM;

机译：主义;丰富— ISM；个人（天鹅环）— ISM；超新星残留物-X射线；主义;

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专利

1. Suzaku observation of the southeastern rim of the Cygnus Loop [J] . Kosugi H., Tsunemi H., Katsuda S., PASJ: Publications of the Astronomical Society of Japan . 2010,第4期

机译：朱雀对天鹅座环东南缘的观测
2. Suzaku Observations across the Cygnus Loop from the Northeastern to the Southwestern Rim [J] . Kimura Masashi, Tsunemi Hiroshi, Katsuda Satoru, PASJ: Publications of the Astronomical Society of Japan . 2009,第sp1期

机译：从东北到西南沿天鹅座圈的朱雀观测
3. JOINT SUZAKU AND XMM-NEWTON SPECTRAL ANALYSIS OF THE SOUTHWEST CYGNUS LOOP [J] . Denis Leahy, Mohammed Hassan The Astrophysical journal . 2013,第1期

机译：西南天鹅环的联合SUZAKU和XMM-Newton谱分析
4. Suzaku Observation of the South-East Limb of the Cygnus Loop [C] . Hiroko Kosugi, Hiroshi Tsunemi, Hiroyuki Uchida, Suzaku international conference on energetic cosmos : from Suzaku to ASTRO-H . 2010

机译：朱雀观察了天鹅座循环的东南肢体
5. The development of the spatial heterodyne spectrometer for observations of C IV emissions near 1500 A from the cygnus loop and the diffuse hot interstellar medium. [D] . Watchorn, Steven Ronald. 2001

机译：空间外差光谱仪的发展，用于观测来自天鹅环和弥漫性星际介质的1500 A附近的C IV发射。
6. Comparative Analysis of the Fecal Bacterial Microbiota of Wintering Whooper Swans (Cygnus Cygnus) [O] . Wenxia Wang, Songlin Huang, Liangliang Yang, 2021

机译：越冬冬孔天鹅（Cygnus cygnus）的粪便细菌微生物的比较分析
7. Suzaku Observations across the Cygnus Loop from the Northeastern to the Southwestern Rim [O] . Masashi Kimura, Hiroshi Tsunemi, Satoru Katsuda, 2008

机译：从东北到西南边缘的天鹅座环路上的朱雀观测
8. Possible Charge-Exchange X-Ray Emission in the Cygnus Loop Detected with Suzaku [R] . Katsuda, S., Tsunemi, H., Mori, K., 2011

机译：用朱雀检测天鹅座环中可能的电荷交换X射线发射

Suzaku Observation of the South-East Limb of the Cygnus Loop

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