Chinese translation for "金属度"

metallicity

Example Sentences:

	1.	Specification for sprayed unfused metal coatings for engineering purposes 工程用喷镀的未熔金属度层规范
	2.	Specification for sprayed and fused metal coatings for engineering purposes 工程用喷涂和熔融金属度层规范
	3.	High - metallicity cluster 高金属度星团
	4.	Low - metallicity cluster 低金属度星团
	5.	It is also pointed out that the " pre - enrichment " ca n ' t be used to explain the bimodal structure of metallicity distribution of gcs 本文的研究同时指出， “预增丰”不可能造成球状星团系统的金属度双峰结构。
	6.	It has long been known from observations that the metallicity distribution of galactic gcs shows bimodal structure . in recent years the same distribution feature has also been found in other galaxies . how to explain this phenomenon is a challenge to the formation and evolution of gcs 观测发现银河系和其它星系中的球状星团系统普遍表现出类似的金属度分布双峰结构，这一分布特征成为研究球状星团形成与演化极为重要的观测约束条件。
	7.	The differences in orbital morphologies due to different potentials is slighting , however , given a certain potential , for clusters that have perigalactic distance smaller than 1 kpc , some orbits may exhibit a chaotic behavior . the correlation between the metallicity of samples and the orbital morphologies is unclearly ; ( 4 ) it is found that the semi - major axis , apogalactic distance and azimuth period of 29 sample clusters are changed with their metallicity similarly , but a obvious correlation is seen between orbital eccentricity and metallicity . there is a fraction of 24 % of the sample clusters with eccentricities lower than 0 . 4 不同的引力势模型对球状星团轨道的具体形态影响不大，在给定的引力势模型下，当某些星团的运动轨道穿越距银心1kpc附近的区域时会出现“混沌”现象： ( 4 ) 29个样本星团的轨道半长轴、远银心距和方位周期随金属度的变化规律基本相似，样本星团的金属度与其轨道形态之间的相关性并不明显，然而轨道偏心率与金属度有关，对于所选的晕族样本星团而言，大约有24的样本星团的轨道偏心率低于0 . 4 。
	8.	The calculating results show : ( 1 ) most of samples are located in 5 kpc - 10 kpc from galactic center . all of the sample clusters present a spherical symmetrical distribution around the galactic center , and their space velocities are presented a ellipsoidal distribution ; ( 2 ) according to the metallicity and basic characters , the sample clusters are separated into hb subgroup and mp subgroup . the number of samples are changed with metallicity [ fe / h ] , and there is a peak at [ fe / h ] = - 1 . 6 ; ( 3 ) the orbits of sample clusters show mostly limited , periodic characteristics , but the orbits are not closed completely , their maximal galactocentric distance is less than 40 kpc 计算结果表明： ( 1 )大部分样本星团都位于银心距5kpc 10kpc的范围内，相对于银心呈球对称分布，它们的速度也呈椭球分布； ( 2 ) 29个样本星团按其金属度大小和基本性质分类，可分属hb和mp两个球状星团次系，且样本星团数随金属度[ fe h ]而变化，在[ fe h ] = - 1 . 6处出现一个峰值； ( 3 )所有样本星团的轨道运动都呈周期性，大都在一个有界而不封闭的周期轨道上运动，其最大银心距都在40kpc以内。
	9.	The high metallicity of disk gcs was caused by the particular environment they are situated . because of the strong interaction wjth the disk , the extent of outflow and star formation efficiency ( sfe ) of the disk gcs was quite different from the halo gcs , which leads to the significant difference between the metallicity distribution of two classes of gcs 本文建立的自增丰演化模型对球状星团的余属度双峰分布提出了一种新的解释，指出盘族球状星团之所以出现较高的金属度，是因为它处于银盘这一特殊的环境下，与银盘相互作用而造成比晕族球状星团更为强烈的增丰。

Similar Words：

"金属镀盖" Chinese translation, "金属镀胶" Chinese translation, "金属镀面" Chinese translation, "金属镀膜磁带" Chinese translation, "金属镀铁硬化" Chinese translation, "金属度梯度" Chinese translation, "金属渡槽" Chinese translation, "金属短路试验" Chinese translation, "金属短纤维" Chinese translation, "金属锻压工" Chinese translation