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1.K-Shell Ionisation of Al and Si Thin Targets by 0.4-3.0 Mev Incident Protons
0.4-3.0Mev质子激发Al和Si薄靶的k-x射线研究收藏指正
2.CHARACTERISTIC K-SHELL X-RAYS PRODUCTION IN Al,Ti AND Ni BY 250 TO 430Kev PROTONS
铝、钛和镍在250—430Kev质子轰击下产生的K层特征X射线收藏指正
3.Four collocation types of damping spring bar applied to K8 single-layer latticed shell structure were introduced. The influence of relieving effect of damping spring bar collocation in the structure and mechanical behavior of damping spring load-relieving latticed shell were analyzed. Furthermore, the influence of the stiffness coefficient K of damping spring bar was discussed.
通过阻尼弹簧杆在K8型单层网中的四种布置形式,讨论了阻尼弹簧杆件布置对荷载缓和效果的影响,并对阻尼弹簧荷载缓和网的受力特性进行了研究,同时探讨了阻尼弹簧杆刚度系数K的影响。收藏指正
4.We present H and K s polarimetric images in a ~5′ field of star forming region NGC7538. The polarimetric images reveal the complex structure of infrared nebulosities and clusters of young stars, associated with the bright infrared sources IRS 1 11. The polarization pattern in the IRS 1 3 nebula shows a dominant illumination from deeply embedded source IRS 1. The morphology of the nebula can be modeled by a low extincted bubble enclosed by redder and highly polarized shell.
介绍恒星形成区NGC7538的H和Ks波段偏振成像的观测结果.近5′视场的偏振图像揭示了与亮红外源IRS1?11成协的年轻星团和红外星云的复杂结构.IRS1?3星云的偏振图像表明星云的近红外辐射主要来自对深埋红外源IRS1的反射;收藏指正
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