- 更多网络例句与超星系相关的网络例句 [注：此内容来源于网络，仅供参考]
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Blazars are one of the most extreme classes of active galactic nucleus, with high luminosity, large amplitude and rapid variability, high and variable polarization, radio core-dominance, and apparent superluminal speeds.
在活动星系核中，Blazar天体是具有极端性质的一类，它以大幅快速光变、高且变化的偏振、射电核主导、视超光速运动、全波段非热辐射为主要特征。
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In the center of NGC 6240, the two black holes in the cores will whip up a frenzy of radiation as they careen towards one another head-on, likely transforming the galaxy into a monster known as an ultra-luminous infrared galaxy, thousands of times as bright in infrared as our Milky Way.
在NGC 6240星系的中心，星系内核中的两个巨大黑洞将激发狂乱的辐射物，加剧两个星系内核的合并进程，很可能会使它们合并成为一个超明亮的红外星系，其红外线亮度是银河系的数千倍。
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The team used FLAMES, the super-efficient spectrograph at ESO's Very Large Telescope at the Paranal Observatory in Chile, to make ultra-precise measurements of a host of planetary nebulae in the outskirts of Messier 87 and in the intergalactic space within the Virgo Cluster of galaxies, to which Messier 87 belongs.
研究团队使用FLAMES——VLT阵列中的超高效摄谱仪，极为精确的测量了M87外缘和室女座星系团星系间空间中的行星状星云。
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The observational study of extragalactic H2O megamaser sources and molecular emission lines associated with AGNs is a very efficient tool to investigate characteristics of certral sources in AGNs and circumnuclear toruses of gases and dusts.
对与活动星系核成协的河外超脉泽源及分子谱线的观测和研究是探测和研究活动星系核核区中央源、拱核气体和尘埃环性质的非常有效的工具。
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The luminosity of the most of extraglactic H2O megamaser sources is between tens and hundreds L ⊙, but one of the extragalactic H2O megamaser source TXFS 2226-184 is 6100 L ⊙. It belongs to the class of radio galaxy and is not general. It is mainly caused by its wide spectral profile.
多数河外H2O超脉泽源的光度在几十至几百个 L ⊙之内，但TXFS2226－184源的河外H2O超脉泽源的光度达6100 L ⊙，它属于射电星系类型，是主要由于其谱线轮廓较宽所造成的一种例外情况。
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Since the first extragalactic H2O megamaser source toward the Active Galactic Nuclei NGC 4945 was discovered, 19 sources have been found.
自从在活动星系核NGC 4945的视线方向上发现第一个河外H2O超脉泽源以来，迄今为止已发现了19个河外H2O超脉泽源。
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Because NGC 4603 is much farther away than the other galaxies studied with Hubble by the Key Project team, 108 million light-years, its stars appear very faint from the Earth, and so accurately measuring their brightness, as is required for distinguishing the characteristic variations of Cepheids, is extremely difficult.
由于它远在1.08亿光年外，远超项目组团队研究的其他星系，故此恒星变得非常黯淡，而任务要求必须正确测定其中的特定变星——造父变星——的光度，显得格外困难。
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The types are the low rider classic bikes, competitor bikes, crown bikes, deluxe bikes, super wheel bikes, twister, fan wheel, galaxy, 3-speed, etc.
的类型是典型的低车手自行车，摩托车的竞争对手，皇冠自行车，豪华摩托车，超轮自行车，捻线机，风扇轮，星系，3速，等
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The telescope snapped images of galaxies in the faraway universe in a series of unique observations: the Hubble Deep Fields, the Great Observatories Origins Deep Survey, the Hubble Ultra Deep Field,and as part of an armada of observatories in the All-wavelength Extended Groth Strip International Survey.
哈勃空间望远镜以一系列独特的视角拍摄了遥远的星系的图像：哈勃深空场，大天文台起源深空巡天，哈勃超深空场，作为国际全波段扩展巡天的一个天文台舰队。
- 更多网络解释与超星系相关的网络解释 [注：此内容来源于网络，仅供参考]
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great attractor：巨引源
1980年代,Faber在进一步研究Faber-Jackson关系时,参与了巨引源(Great Attractor)的发现,这是个驱动包括银河系在内大量星系运动的引力源,属于超星系团.
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red shift, distances：红移、距离
9850G 星系的辐射和光谱 radiation and spectra of galaxies | 9850H 红移、距离 red shift, distances | 9850K 星群、星团、超星团 groups, clusters, superclusters
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Sculptor group：玉夫星系群
scroll 卷滚 | Sculptor group 玉夫星系群 | Sculptor Supercluster 玉夫超星系团
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Sculptor Supercluster：玉夫超星系团
Sculptor group 玉夫星系群 | Sculptor Supercluster 玉夫超星系团 | Sculptor void 玉夫巨洞
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supergalactic streamer：超星系流状结构
supercluster 超星团; 超星系团 | supergalactic streamer 超星系流状结构 | superhump 长驼峰
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Blobs：斑点
因此,天文学家最近发现,七个以上的似星体喷出斑点(blobs)物之移动速度比光速还快,将如何解释?就当作光的幻觉吧!这七个新找到的超亮物体,也会引发我们构想新的观点;那是有关会发出强烈电波的星系核心及似星体所产生的巨大动力,
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supergalaxy：超星系
超银经 supergalactic longitude | 超星系 supergalaxy | 超巨星 supergiant
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local supergalaxy：本超星系
local supercluster ==> 本超星系团 | local supergalaxy ==> 本超星系 | local supplies ==> 当地料源,地方资源