The environment near SNR W41 and W30

30.06.2013 • Views

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The environment near SNR W41 and W30

The environment near SNR W41 and W30

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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

The Evolution & Structure of Pulsar Wind Nebulae

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

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Page 1 and 2: The environment near SNR W41 and W3
Page 3 and 4: W41
Page 5 and 6: XMM-Newton observation 0.3-1.5keV 1
Page 7 and 8: Chandra map Zoom in Misanovic et al
Page 9 and 10: SED of W41 GeV break GeV-TeV break
Page 11 and 12: W30 complex •SNR G8.7-0.1 (W30)
Page 13 and 14: X-rays in the field of W30 •PSR B
Page 15 and 16: GeV break GeV-TeV break
Page 17 and 18: Possible explainations •PWN? high
Page 19: SNR-MC • One cloud or two clouds?