Mira variables

AM the selected OH/ IR sources have optical or infrared identification. Most of them are associated with late-type (> M5) Mira variables.

所选127个OH/IR脉泽源全部是有光学或红外证认的，其中大部分是光谱型>M5的长周期变星（主要是Mira变星）。

The Two-Fluid Model of The Velocity Fields of the Circumstellar Envelop of Mira Variables

Mira变星拱星包层速度流场的二流模型

For typical Mira variables we made numerical calculations and obtained a temperature curve.

对于典型的Mira变星我们进行了数值计算，得到了温度曲线。

The Velocity Fields of Axial-Symmetrically Rotating and Expanding Circumstellar Envelopes of Mira Variables

Mira变星的有轴对称转动膨胀的拱星包层速度流场

A further discusses concerning the mass loss rates from Mira variables

关于Mira变星质量损失率的进一步讨论

The Temperature Structure of the Circumstellar Envelopes of Mira Variables

Mira变星拱星包层的温度结构

The mass loss rates and sound point positions. for an adiabatic expanding process from Mira variables

Mira变星的绝热膨胀过程的质量损失率和声点半径