查询词典 Cor tauri

When the moon departs from the evening sky in a few more weeks, you should have no trouble seeing Zeta Tauri from a dark country sky.

数周之后，当月亮不在天空中出现时，你就可以毫不费劲的找到Zeta Tauri 。

To further complicate the picture, infrared observations indicate that T Tauri itself is part of a multiple system and suggest that the associated Hind's Nebula may also contain a very young stellar object.

红外光波段的观测更雪上加霜让情况更加复杂难解，因为结果显示金牛座T星是一个多合星系统的成员，而和它相关的海德变光星云本身可能也藏有一个非常年轻的星体。

HOURS, MAY 1, 2531 \ 111 TAURI SYSTEM, CAMP NEW HOPE, PLANET VICTORIA

军历2531年5月1日1647时 \ 111陶利星系，新希望营地，维多利亚星

I followed the monthly pulsations of T Monocerotis, the unpredictable quiverings of Y Tauri, and the nightly creep of asteroids.

在那儿，我跟踪麒麟座T 每个月的脉动，金牛座Y 不可预言的亮度变化，以及小行星的缓慢移动。

The rather faint star Zeta Tauri pinpoints the tip of the Bull's southern horn, but the glary moon will make this star difficult if not impossible to see tonight.

光芒黯淡的Zeta Tauri 却能准确的指出位于南部天空的牛角尖，但是由于月亮强烈的光芒，今夜我们会很难找到这颗星星。

Over 400 light-years away, at the edge of a molecular cloud , both star and nebula are seen to vary significantly in brightness but not necessarily at the same time, adding to the mystery of the intriguing region. T Tauri stars are now generally recognized as young -- less than a few million years old -- sun-like stars still in the early stages of formation .

它们的 观测亮度会有大幅度的变化，不过不一定会同步，而这也是此区域的谜团之一。T型变星通常是年龄不到数百万年的年轻类太阳恒星，还处在恒星形成的初期阶段。

The theory of accretion disks are important for many astrophysical phenomena, including Quasars, active galatic nucleic, X-ray binary stars, and young stellar objects. The most important branch of accretion djsk theory is the stability properties of djsks. It is widely considered that the luminosity variations of various astronomical objects are associated with the instability of accretion disk. The viscosity plays an important role in the accretion disk theory, and magnetic field exists commonly in astronomical phenomena. A more realistic analysis of the stabihty of the accretion disk should include both the radjal and azimuthal perturbations because of the strong shear of viscous flow.In this paper, according to the luminosity Variations of Various astronomical objects, we study the radial-azimuthal instability of an isothermal with magnetic field. We find that the radial and azimuthal fields B〓,B〓 are mainly responsible for enhancing the instability of the magneto-acoustic modes and non-axisymmetric modes,and that pulsational oscillations are larger in the radial than in the Z direction. The model may be useful in explaining the periodic light variation of FU orionis and. T Tauri stars.

在许多天体物理现象中，例如活动星系核，X-射线双星和年青的恒星理论中，吸积盘理论起着重要的作用，而吸积盘理论中的一个重要分支是吸积盘的不稳定性理论，普遍认为活动天体的周期，准周期光变现象与吸积盘的不稳定性有关，在吸积盘理论中，粘滞起着重要的作用，而磁场是天体物理中普遍存在的现象，对于几何薄吸积盘不稳定性分析，由于强剪切流的缘故，应该包括径向和环向扰动两个方面，本文结合天体物理中的各种周期，准周期光变现象，研究了含磁场的等温薄吸积盘的径向-环向振荡不稳定性，结果表明：磁场的径向和环向分量对磁声模和非轴对称模的不稳定性的增加起着主要的作用，且径向振荡大于轴向振荡，所得结果有利于解释FU Orionis和T Tauri Stars的周期光变现象。

Astronomers John Carr of the Naval Research Laboratory in Washington, D.C., and Joan Najita of the National Optical Astronomy Observatory in Tucson, Arizona, used Spitzer to tease out the signals revealing the molecular composition of the gas in the disk surrounding AA Tauri, a star less than a million years old located in the constellation Taurus.

华盛顿哥伦比亚特区海军研究实验室的天文学家约翰·卡尔，和亚利桑那州图森国家光学天文台的天文学家琼·纳吉塔，利用斯必泽太空望远镜挑选出能够揭示恒星" AA 托莱"周围圆盘中气体分子构成情况的信号。恒星" AA 托莱"位于金牛座，诞生于不到一百万年前。

Young variable star RY Tauri is emerging from a yellowish cocoon of dust near top center.

图中正上方，年轻的金牛座变星——金牛座RY从泛黄的尘埃茧中露出头来。

In 2 Cor 1:5 he tells us that Christ's sufferings abound in us.

在哥林多后书1：5他告诉我们多受基督的苦楚。

"Second Life is remarkably easy to work with, and is very popular,"

"第二次生命是显着容易的工作，并且很受欢迎，"

For example, we usually assume that materials are homogeneous and isotropic and free of internal defects or flaws.

为了得到适合有限元分析的模型，我们必须经过如图2所示的简化步骤。