共查询到20条相似文献,搜索用时 15 毫秒
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Carter LJ 《Science (New York, N.Y.)》1967,157(3795):1413
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Ney EP 《Science (New York, N.Y.)》1977,195(4278):541-546
Infrared astronomy has shown that certain classes of stars are abundant producers of refractory grains, which condense in their atmospheres and are blown into interstellar space by the radiation pressure of these stars. Metallic silicates of the kind that produce terrestrial planets are injected by the oxygen-rich stars and carbon and its refractories by carbon stars. Much of the interstellar dust may be produced by this mechanism. A number of "infrared stars" are completely surrounded by their own dust, and a few of these exhibit a unique morphology that suggests the formation of a planetary system or a stage in the evolution of a planetary nebula. Certain novae also condense grains, which are blown out in their shells. In our own solar system, comets are found to contain the same silicates that are present elsewhere in the galaxy, suggesting that these constituents were present in the primeval solar nebula. 相似文献
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以棉花品种鄂抗棉-10和铜杂411为研究对象,对棉花幼苗进行不同加载速度下的剪切和弯曲试验,并对钵体进行压缩试验。结果表明:不同品种棉花幼苗的剪切强度和弯曲强度都随加载速度的增大而增大;在相同加载速度下,鄂抗棉-10的剪切强度和弯曲强度均大于铜杂411;对剪切强度和弯曲强度进行可重复双因素方差分析,结果表明加载速度和品种对棉花幼苗的剪切强度和弯曲强度均有显著影响,两者的交互作用对剪切强度和弯曲强度无显著影响。钵体在径向和轴向压缩方式下的破裂力分别为73.3~110.5N和100.3~192.3N,钵体的抗挤压能力具有各向异性。 相似文献
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