The Evolution & Structure of Pulsar Wind Nebulae

30.06.2013 • Views

Share Embed Flag

The Evolution & Structure of Pulsar Wind Nebulae

The Evolution & Structure of Pulsar Wind Nebulae

DOWNLOAD ePAPER

astronomy.nju.edu.cn

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

START NOW

G320.4-1.2<br />

2

X-ray nature of the LINER nuclear sources

第五章星际介质和恒星形成

第八章活动星系

Kuiper

彗星运动中的混沌运动

Jiangtao Li

中等质量X射线双星的演化 - 南京大学天文系

第三章回归分析

星际尘埃的性质和观测研究

Be/X射线双星的多波段研究

第三体摄动的摄动函数展开

The Interactions between the SNRs and Their Environments

Chandra X-Ray Observatory

彗星 - 南京大学天文系

G320.4-1.2 2

Wisp ACIS-S3 (11/3/2000- 4/6/2001) v ~ 0.5c (Heter et al. 2002) (Koji Mori, 2002) 2

Page 1 and 2: The Evolution & Structure of 2007-0
Page 3 and 4: • SNR => pulsar-driven SNR => PWN
Page 5 and 6: Theoretically Theoreticall • Marv
Page 7 and 8: Pulsar Wind-magnetodynamic Wind mag
Page 10 and 11: Emission & Spectra of nebulae • T
Page 13 and 14: Evolution • Phase I - Expanding i
Page 15 and 16: Phase I 1
Page 20: Torus, Jet, Wisp & Filament 2
Page 24: • G54.1+0.3: luminosity, geometry
Page 29 and 30: • Optical: Filaments - R-T instab
Page 31 and 32: Filaments • X-ray filaments of 3C
Page 33 and 34: Phase II Phase III 3
Page 35 and 36: Phase II Phase III 3
Page 37 and 38: Phase III Phase IV 3
Page 39: Other & Recent results • Very you