thick disk的例句大全

New Progress in Chemical Abundance of Galactic Thick Disk Stars

银河系厚盘恒星元素丰度研究

The Thick Disk of the Milky Way Galaxy and its Formation Mechanisms

银河系厚盘及其形成机制

Age-Metallicity Relation of Stars in the Galactic Thick Disk

银河系厚盘恒星的年龄-金属度关系

A comprehensive study in stellar elemental abundances, age and kinematics will be able to refine and constrain various models of Galactic thick disk formation.

结合年龄、运动学参数研究，恒星元素丰度可以对银河系厚盘形成机制提供观测依据。

Under the high-frequency, high power sound radiation conditions, the mechanical strength of thin disk get insufficient. Then the thick disk is a good choice because it possesses advantages of small transverse dimension and high frequency.

在高频、大功率声辐射条件下，薄盘的机械强度显得不足，这时厚圆盘是个不错的选择，因为它横向尺寸不大，频率又高。

Recent observations show that the abundance patterns of α-elements in the thin and thick disk are distinct, and this difference also appear for some other elements, such as Al, Mn, Zn and neutron-capture elements.

近年来很多工作发现，厚盘恒星的α元素丰度随金属丰度的变化趋势与薄盘不同，这种不同还表现在Al、Mn、Zn、中子俘获元素等其他元素上。

A Model of Thick Accretion Disk of QSOs with Magnetic Field

类星体的有磁厚吸积盘模型

The thick accretion disk model with a QUASI-DIPOLE magnetic field

具有类偶极磁场的厚吸积盘模型

The Thick Accretion Disk Model and Self-gravitating Accretion Disk Model of QSOs

类星体的厚吸积盘与自引力吸积盘模型

As a result, 15 W output power at 1.03 μ m with a slope efficiency over 40% from a 0.35 mm thick Yb ∶ YAG disk laser is obtained.

用0.35mm厚的Yb∶YAG薄片获得15.9W的1.03μm激光输出，斜率效率超过40%。

The general shape of the average nebula is that of a thin circular disk somewhat thick in the center.

星云最常见的形状是中间较厚边缘较薄的圆盘。

Fabrication and Finite Element Analysis of Piezoelectric Thick-Film Micro-Actuator for Hard Disk Drives

硬盘用压电厚膜微致动器的制作及有限元分析

under normal molding conditions, where would the most volumetric shrinkage occur on a center-gated, flat, and uniformly thick round disk?

在通常的成型条件下，一块具有中心的、平的、均匀的厚的圆盘在什么地方收缩最大？

petals oblong. disk thick, cupulate.

花瓣长圆形花盘厚，杯状。

disk thick, fleshy, 5-lobed, distinctly emarginate in front of stamens, outer margin prominent.

花盘厚，肉质，5浅裂，在雄蕊的前面清楚微缺，外部边缘突出。

petals obovate. disk pentagonous, thick.

花瓣倒卵形花盘五角形，厚。

The Thick Accretion Disk Model and Self-gravitating Accretion Disk Model of QSOs.

类星体的厚吸积盘与自引力吸积盘模型.

The radiation pressure supported thick accretion disk model has been studied more extensively, and it seems to have some difficulties.

辐射压支持的流体厚吸积盘模型已经得到比较多的研究，看来存在一些难以解决的问题。

The conclusion is: the short term variability behavior provides a strong support to the thick accretion disk model of AGN.

这些讨论表明，活动星系核的短时标光变特征对厚吸积盘模型提供了强有力的支持。