1.
Spectral Line Observations of Massive Star Forming Regions and Circumstellar SiO Maser;
大质量恒星形成区和恒星SiO脉泽的谱线观测研究
2.
TENDENCY TO CLUSTER IN MASSIVE STAR FORMATION
大质量恒星形成时的成团倾向(英)
3.
Massive stars are hottest in their central regions.
大质量恒星的中心区域温度最高。
4.
In theory, the first step toward producing a millisecond pulsar is the formation of a neutron star when a massive star goes supernova.
理论上，形成一颗毫秒脉冲星的第一步，是一个大质量恒星在成为超新星而爆发后留下的中子星。
5.
The disrupted sunlike star could form a massive disk in orbit around the dwarf.
瓦解的类太阳恒星可能在环绕白矮星的轨道上形成一个质量巨大的盘状物。
6.
Hot bluish white clusters of massive stars are scattered throughout the galaxy, interspersed with numerous dustier reddish regions of current star formation.
炽热的蓝白色大质量恒星群遍布整个星系，散布在众多充满尘埃略带红色的恒星诞生区中。
7.
Rocky planets would form nearest the parent star, with gas giants farther out.
石质行星会在靠近起源恒星的区域形成，而气态的巨行星在外围形成。
8.
High-mass stars emit ultraviolet and blue light, whereas low-mass stars emit yellow and red light.
大质量恒星发出紫外光和蓝光，而小质量恒星则发出黄光与红光。
9.
Stars are born from a kind of primal soup known as the interstellar medium.
恒星是由一种称为星际介质的“原汤”形成的。
10.
Accretion Disk and Angular Momentum Loss During Formation of a Star in the Nebular Disk
吸积盘与恒星在星云盘中形成时的角动量损失
11.
The black hole could then grow even stronger (from the star's mass) as to possibly absorb another.
吸收了恒星质量之后，黑洞进一步膨大，并有可能吞噬下一颗恒星。
12.
Black holes are the evolutionary endpoints of stars at least 10 to 15 times as massive as the Sun.
黑洞是恒星演化的终点，这些恒星的质量通常有10－15个太阳大
13.
The answer is crucial to understanding the processes at play in low-mass stars and giant planets and the differences between them.
这个答案对于理解低质量恒星和巨行星的形成过程，以及它们之间的差异，至为关键。
14.
The material drawn tidally from the large dying star thus forms a tail that chases the denser companion star from behind.
于是，从大的垂死恒星如潮汐般涌出的物质，便形成了一条尾巴，紧追在致密伴星之后。
15.
This circumstance means that cool molecular gas is located there, a vestige of the original gas-dust cloud from which not massive stars were formed, spawning HII zones.
这种情形意味着那里有冷分子气体，它是形成大质量高温星、产生HⅡ区的原始气尘云残余。
16.
Thick clouds of interstellar gas absorb most of the light and screen other stars from us.
恒星间气体所形成的厚云层，吸收大部分的光，并遮住其他星星。
17.
The diameters of stars, unlike their masses, have an enormous range.
恒星的直径不同于它们的质量，相差很大。
18.
The regions of greatest metal enhancement for a given star-forming frequency apparently suffer the greatest compression.
对于一定的恒星形成频率，金属加浓最大的区域显然受到了最大的压缩。