- 更多网络例句与原恒星相关的网络例句 [注：此内容来源于网络，仅供参考]
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A number of sourceless cores, UC HII regions and their physical parameters were obtained. Initial conditions of masive star formation were inspected. This provided samples for further larger observations.
对用MSX、IRAS选取的一批样品进行CO及其同位素成图观测研究，获得了无源云核、原恒星云核及UC HII区云核及其物理参量，考察大质量恒星形成初始条件，同时为更大规模脉泽观测准备样品。
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As a result, some theorists propose that massive stars must form from collisions of smaller protostars.
因此有些理论家提出大质量恒星必定起源于较小的原恒星之间的碰撞。
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There are two forces that counteract gravity to suppress the fragmentation of the cloud: thermal pressure from the heat of protostars, and turbulence, which may allow massive stars to form directly from accretion.
有两种力可以抵消引力的作用从而抑制星云的破碎：源于原恒星热量的温压，以及湍流--它可能允许大质量恒星通过吸积直接形成。
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Simple laws of physics suggest, that gas-dust complexes in the interstellar medium may evolve, first into protostars and subsequently into stars.
简单的物理学定律揭示出，星际介质中的气尘复合体可以进化，先是演化为原恒星，接下去再演化为恒星。
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Simple laws of physics suggest, that gas-dust complexes in the interstellar medium may evolve , first into protostars and subsequ tly into stars.
简单的物理学定律揭示出，星际介质中的气尘复合体可以进化，先是演化为原恒星，接下去再演化为恒星。
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These dust and gas clouds lie near the edge of a large molecular cloud. Themselves telltale signs of star-forming regions, they tend to hide the newly formed stars and young stellar objects or protostars from prying optical telescopes.
这些尘埃与氢气云都位在一个大分子云的边缘，而它们本身也是恒星诞生区的标志，不过对光学望远镜观测来说，它们也是遮掩新生恒星和原恒星的障碍。
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Their simulation of the birth of a protostar in the early universe signifies a key step toward the ambitious goal of piecing together the formation of an entire primordial star and of predicting the mass and properties of these first stars of the universe.
他们对早期宇宙中原恒星诞生的模拟是一个重要进展，该研究的最终目标是对一个完整的原恒星的形成做全面描述，并且预测宇宙中第一批恒星的质量和属性。
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According to their simulation, gravity acted on minute density variations in matter, gases, and the mysterious "dark matter" of the universe after the Big Bang in order to form this early stage of a star -- a protostar with a mass of just one percent of our sun.
根据他们的模拟，大爆炸之后，引力对宇宙中的物质、气体和神秘的&暗物质&起作用使其分布密度产生变化，从而形成原恒星状态——形成的原恒星质量只有太阳的1%。
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The result is a detailed description of the formation of a protostar -- the early stage of a massive primordial star of our universe -- and the researchers' computer simulation, which has been called a "cosmic Rosetta Stone," sets the bar for further investigation into the star formation process.
这篇文章详细描述了原恒星的形成过程——它们是宇宙中大质量原始恒星的早期状态，他们称之为&宇宙罗塞塔石碑&的计算机模拟程序目的是要对恒星的形成过程做深入研究。
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Dr. Yoshida's simulation also shows that the protostar would likely evolve into a massive star capable of synthesizing heavy elements, not just in later generations of stars, but soon after the Big Bang.
另外，Yoshida博士的模拟也揭示了原恒星演化成大质量恒星的可能性，在大质量恒星中一些较重的元素得以合成，模拟背景不是原恒星的后续演化，而是在大爆炸之后。
- 更多网络解释与原恒星相关的网络解释 [注：此内容来源于网络，仅供参考]
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Musca：苍蝇座
天文学家在猎户座 (Orion)也发现了许多称为原行星 (proplyds)的行星形成系统. 这些恒星系统中刚在形成的行星,要能够承受周围亮星强烈辐射的洗礼,才能成为一颗颗真正的行星. HD 100546位在南天的苍蝇座 (Musca),距离我们只有335光年,用双筒望远镜就能看到它.
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proper motion star：大自行恒星
proper motion in right ascension 赤经自行 | proper motion star 大自行恒星 | proper time 原时
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subatomic particles：亚原子粒子
proto-stellar clouds 原恒星云 | subatomic particles 亚原子粒子 | antimatters 反物质
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sunlike star：类太阳恒星
protoplanetary disk原行星盘 | sunlike star 类太阳恒星 | transit 凌星
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protostar：原恒星
Torres 上尉发现刚传送上船的原恒星 (Protostar) 样本出现了异状;一个样本罐里有物质,另一个则是空的. 再重新传送后,修正了这个异状. Torres上尉告知 Janeway 舰长她需要执行 6 个小时的光谱分析,并推断如果善加运用的话,