thick disk

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 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 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.

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 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 Disk of the Milky Way Galaxy and its Formation Mechanisms

银河系厚盘及其形成机制

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。

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。

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。

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

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 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。

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。