- 更多网络例句与伴星相关的网络例句 [注：此内容来源于网络，仅供参考]
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In this scenario, a neutron star in a binary system can accrete matter from its companion.
一个双星系统中的中子星会从伴星处吸积足够物质，使得该中子星最后变成了一颗奇异星。
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Several explanations have been proposed, including cycles of magnetic activity somewhat similar to our own Sun's sunspot cycle, the action of companion stars orbiting around the dying star, and stellar pulsations.
现在有几个被提出的解释，包括像我们自己的太阳黑子周期的磁场周期活动，围绕衰老的恒星轨道有规律运动的伴星。
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In 1862 Alvan Graham Clark discovered the companion, which is called Sirius B, or affectionately "the Pup".
在1862年Alvan Graham Clark发现了伴星，它被称作天狼星B，或亲切地称为"小子"。
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It was supposed that Sirius must be affected by a second star, and in 1862 a faint companion star was finally detected by Alvan Clark, and it was named Sirius B.
据猜测天狼星一定受到第二颗星作用影响，而在1862年Alvan Clark发现一颗暗淡的伴星，就把它取名为天狼星B。
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Part of a binary star system, the compact white dwarf gradually captured material from its companion star.
作为一个双星系统的一部分，这颗致密的白矮星慢慢地从它的伴星上吸积物质。
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Also known as Messier 51a, M51a, or NGC 5194, the Whirlpool Galaxy is an interacting grand-design spiral galaxy located at a distance of approximately 23 million light-years in the constellation Canes Venatici.
漩涡状星系又被称为"梅赛耶51a"，"M51a"或"NGC 5194"，与的地球距离为2300万光年，位于北天的猎犬座，是一个庞大的，与它的伴星系共存的螺旋状星系。
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Its companion star is diagonally above it at 10 o'clock.
它的伴星则位于上方10点方向。
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In general, Ba stars belong to binary systems, and their heavy-element overabundances are due to the accreting material from the companions (the former TP-AGB stars and the present white dwarfs).
一般认为它们属于双星系统，其伴星已经经历了AGB阶段，Ba星也就因此而吸积了其伴星抛出的富含重元素的物质。
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In general , ba stars belong to binary system , and their heavy - element overabundances are due to the accreting material from the companions ( the former tp - agb stars and the present white dwarfs ). carrying out a series of monte - carlo simulations , the changes of orbital elements of binaries are recalculated for wind accretion scenario of the total angular momentum conservation
研究表明，钡星应该属于双星系统，其重元素超丰来自双星吸积，它的伴星已经经历了s -过程核合成，而且由在以前发生的同其伴星(以前是agb星，现已演化为白矮星)的质量传输过程中，从伴星那里获得了富含重元素的物质，这样造成了钡星的重元素超丰。
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One possibility is that the central star of Mz3 has a closely orbiting companion that exerts strong gravitational tidal forces, which shape the outflowing gas.
一种可能性是Mz3中心的恒星有一个很近的伴星，这个伴星有着很强的潮汐力，将外流的气体成为特殊形状。
- 更多网络解释与伴星相关的网络解释 [注：此内容来源于网络，仅供参考]
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comes：伴星;伴引血管
comers and goers | 来来往往的人 | comes | 伴星;伴引血管 | comestible | 可吃的 食物
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compact group：紧致群
compact galaxy 致密星系 | compact group 紧致群 | companion 伴星
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companion ladder：升降口梯
companion ladder 舱室扶梯 | companion ladder 升降口梯 | companion star 伴星
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companion：伴星
地球 (Earth) 地地 球球 ((EEaarrtthh))地球是离太阳第三近的行星,轨道半径为14,960 万公里,直径12,756.3 公里,3753(1986 TO)的复杂轨道与地球相关,但不算地球的卫星,视为伴星(companion)月球 (Moon)月月 球球 ((MMoooonn))月球是地球唯一 的卫星,
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planetary companion：类行星伴星
planetary astronomy 行星天文[学] | planetary companion 类行星伴星 | planetary configuration 行星动态
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secondary cosmic radiation：衍生宇宙线
伴星 secondary component | 衍生宇宙线 secondary cosmic radiation | 次起伏 secondary fluctuation
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Vapor deposition：气相沉积
比如有人认为它们源于超新星爆发,有人认为是从富碳巨星(C rich giant)而来,有人则认为它们来自宇宙中的气相沉积(vapor deposition),还有人认为他们是双星系统中的白矮星从富碳伴星吸收了物质之后爆发成超新星的产物.
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electron gas：电子气
(P.A.M.Dirac)将统计力学定律应用于电子气(electron gas)时,理学中. R.H.福勒(Fowler)利用费米-狄拉克气体定律阐明了类似天狼星的伴星这种高密度恒星的结构. 通常称之为白矮星(white dwarfs)的前由G.P.克尤帕尔(Kuiper)所发现的一颗恒星,
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local group of galaxies：本星系群
接近银河星系的星系约30座,叫做"本星系群"(local group of galaxies). 以银河星系为中心,以200万光年为半径,在这空域内一切星系都属于"本星系群",除银河星系外,尚有大、小麦哲伦云及仙女星系. 后者有7个伴星系,其中最大的伴星是M33. 银河阻隔我们的视线,
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neutron star：中子星, Japanese-中性子星
脉冲星pulsar | 中子星, Japanese-中性子星 neutron star | 伴星 companion star