Be/X射线双星的多波段研究

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Be/X射线双星的多波段研究

Be/X射线双星的多波段研究

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Pole ‐on<br />

45 o<br />

Edge‐on<br />

0R *<br />

10R *<br />

From disks to rings<br />

20R *<br />

30R *<br />

40R *<br />

Rivinius et al. (2001) & Meilland et al. (2006)<br />

50R *<br />

60R *

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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

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

Pole ‐on 45 o Edge‐on 0R * 10R * From disks to rings 20R * 30R * 40R * Rivinius et al. (2001) & Meilland et al. (2006) 50R * 60R *

phabs(1)*(gaussian(1)+gabs(1)*cutoffpl(1))*constant(Isis_Active_ Dataset)*cyclabs(1)

Page 1 and 2: Be/X射线双星的多波段研究
Page 3 and 4: Be星 •Hα:形成在7-19R*之间
Page 5 and 6: Be/X射线双星的三种X射线辐
Page 8 and 9: Corbet图 P P spin orb ≤10s ≤ 4
Page 18 and 19: F‐statistic=156.7 for the real da
Page 20: Porb=111.1d Pspin=103s e= 0.47 d=2k
Page 26 and 27: X Persei Porb=250.3d Pspin=837s e=
Page 28: 4U 0115+63 Porb=24.3d Pspin=3.6s e=