1.
Such configurations, obtained theoretically by calculation, are called models of a star.
通过理论计算得到的恒星结构称为恒星模型。
2.
Building model stars is a compulsory task.
建立恒星模型是一项势在必行的任务。
3.
It would be unfair to claim that calculation of model stars inherently contains an element of arbitrariness.
认为恒星模型的计算必然带有某种主观随意性是不公正的。
4.
THE EVOLUTIONARY TRACK IN THE H-R DIAGRAM OF MODEL STARS OF 1.2 SOLAR MASS
1.2 太阳质量的模型恒星在赫-罗图上的演化程
5.
Reynolds Stress Model and Its Helioseismological Testing;
恒星对流的Reynolds应力模型及其日震学检验
6.
The Influence of metal abundant on structure and evolution model of rotating stars;
金属丰度对转动恒星结构与演化模型的影响
7.
Effects of Enrofloxacin on Human Intestinal Mocrofloa in Chemostat Model
低浓度恩诺沙星对离体恒化器模型中人体肠道菌群的影响
8.
A typical globular cluster has about 1 million stars.
一个典型的球状星团包含1百万恒星。
9.
The supernova Ia ratio in milky way galaxy;
银河系Ⅰa型超新星所占星系恒星数目比例
10.
Solar-like Activities in Late-type Stars: ( Ⅰ ): Starspots, Stellar Activity Cycles and Magnetic Field
晚型恒星中的类太阳活动(Ⅰ):恒星黑子、活动周和磁场
11.
On the basis of stellar radial and transverse veloctites, a three dimensional kinematic model has been established for analyzing the local kinematics of the Galaxy in the solar neighbourhood.
利用恒星视向速度和横向速度资料，建立银河系三维运动学模型，以研究银河系在太阳附近运动。
12.
In this model, the resulting implosion and ensuing explosion would blow off the outer envelope of the star and leave behind the core as a neutron star.
按此模型，引起的突然压缩和随后的爆发会把恒量的外部包层吹跑，留下的核成为一颗中子星。
13.
Smaller groups of stars called globular clusters often surround spiral galaxies.
称作球状星团的小型恒星团体经常环绕在旋涡星系周围。
14.
These stars are sometimes called poulation II stars.
这些恒星有时称为星族Ⅱ恒星。
15.
Extrinsic AGB Stars on Wind Accretion Binary Evolution Model
星风吸积双星演化模型下的外赋AGB星
16.
dispersion ring
弥散环 -恒星运动
17.
Conversely, the same processes can actually amplify star formation in large galaxies.
相反的，相同的过程在大型星系中却能增强恒星的形成。
18.
The Turbulence Processes of Stellar Convection and Its Effects on the Oscillation of a δ Scuti Star;
恒星湍对流过程研究以及在盾牌座δ型变星中的验证