星系體 的英文怎麼說

中文拼音 [xīngxìtǐ]
星系體 英文
galaxoid
  • 星 : 名詞1 （夜晚天空中閃爍發光的天體） star 2 [天文學] （宇宙間能發射光或反射光的天體） heavenly body...
  • 系 : 系動詞（打結; 扣） tie; fasten; do up; button up
  • 體 : 體構詞成分。
  • 星系 : [天文學] galaxy; galact-
  1. Although andromeda galaxy is faint for the naked eye, it is one of the farthest objects which can be seen with the unaided eye

    雖然仙女座大星系晦暗難辨，但它可是人類肉眼所能看見最遙遠的天體之一。
  2. In some binary star systems, gas escapes from one star and is captured by the gravity of the other to form a disk

    某些雙星系統中，當從一個恆星逃出的氣體被另一個星體的重力捕獲時，也會形成盤狀結構。
  3. At the current epoch in galactic history, star formation appears to take place in dark-cloud complexes.

    在星系發展的現階段，恆星的形成看來是在暗雲復合體內進行的。
  4. In the conventional view of structure formation, the cluster gas was heated purely by gravitational collapse

    關于結構形成的傳統觀點認為：星系團氣體純粹是經由重力塌縮而加熱。
  5. On the bases of the galaxy evolution theory, we use the therotical chemical evolution model of three zone ( such as halo, thick disk and thin isk ) and multi - phase ( diffuse gas, molecular clouds, stars of both low and high mass, the remnants ). by comparing with the observational constraints, such assurface densities, age - metallicity relation, g - dwarf metallicity distribution in the solar neighbourhood and the correlation between [ a / fe ] and [ fe / h ], supernovae rates, infall rates. the rationality of the model is verified. based on the theory model, we calculate the abundance of neutron capture element

    本文正是在銀河系化學演化的基礎上，利用銀河系的三成分（ threezone ） （即暈、厚盤和薄盤）多相（ multi - phase ） （氣體，分子云，大、小質量恆星以及剩餘物質）的化學演化的理論模型，通過與觀測約束（質量面密度、場星的年齡-金屬豐度關系、太陽附近g矮星金屬含量分佈函數、三成份的特徵量、元素的星系化學演化、超新星的爆炸率、內落速率等）的比較，來檢驗模型的合理性。
  6. The inner part of the galaxy rotates somewhat like a solid wheel, and the arms trail behind

    星系中心部分轉起來有些像一個固體的輪子，旋臂緊跟在後面。
  7. As gas pools, it turns into stars, whose outflows and explosions push material back out into intergalactic space ? a process of negative feedback

    當氣體集中形成恆星，所產生的噴流與爆炸會將物質向外推回星系際空間，這是一種負向的反饋機制。
  8. If the milky way has a very extended corona ( much bigger than the one proposed by spitzer ), this corona could strip off gas from the magellanic clouds

    假如銀河系有一個非常大的星系冕（遠遠大於史畢哲所想像的） ，則它將可拉扯出麥哲倫雲的氣體。
  9. The starts were formed from gases that originally permeated the whole galaxy.

    恆星是由原來遍及於整個星系內的氣體所形成。
  10. The story begins with a local eddy in the swirling gas and dust of the primordial galaxy.

    話題要從原始星系的旋渦氣體和塵埃形成的一個局部渦流說起。
  11. A radio galaxy is related to, but appears larger than, a quasar

    一個射電星系與之有關，但是它比類星體要大。
  12. New stars are constantly forming out of gas and dust in spiral galaxies

    在旋渦星系中不斷由氣體和塵埃形成新的恆星。
  13. Smaller groups of stars called globular clusters often surround spiral galaxies

    稱作球狀星團的小型恆星團體經常環繞在旋渦星系周圍。
  14. These basic system are referred to as radiating, harp, fan, and star systems.

    這些基本體系歸類為：輻射形，豎琴形、扇形和星形體系。
  15. The hot gas will be heated further by any supernova which go off in the galaxy.

    熱氣體將被星系中爆發的任何超新星進一步加熱。
  16. Based on the theoretic research above, a prototype system of multidisciplinary synthetic design for system design of satellite is developed. practice indicates that the synthetic integration of mission analysis stage, system design argumentation stage and system design stage in the whole course of system design of satellite is basically implemented with this system, which offers an assistant tool of design and decision - making for the design staff

    實踐表明，該原型系統基本實現了衛星總體方案設計中任務分析階段、總體方案論證階段和總體方案設計階段全過程的綜合集成，為設計人員提供了一個輔助設計分析、決策的工具;通過系統的開發，探索了一條開展衛星總體多學科綜合設計優化的技術途徑，實踐證明這條思路整體上是可行的。
  17. Topics include : planets, planet formation ; stars, the sun, " normal " stars, star formation ; stellar evolution, supernovae, compact objects ( white dwarfs, neutron stars, and black holes ), plusars, binary x - ray sources ; star clusters, globular and open clusters ; interstellar medium, gas, dust, magnetic fields, cosmic rays ; distance ladder ; galaxies, normal and active galaxies, jets ; gravitational lensing ; large scaling structure ; newtonian cosmology, dynamical expansion and thermal history of the universe ; cosmic microwave background radiation ; big - bang nucleosynthesis

    課程的主題包含了：行星、行星形成；恆星、太陽、正常的恆星、恆星形成；恆星演化、超新星、緻密天體（白矮星、中子星及黑洞） 、波霎、雙x -射線源；星團、球狀及疏散星團；星際介質、氣體、塵埃、磁場、宇宙射線；距離階梯；星系、正常及活躍星系、噴流；重力透鏡；大尺度結構；牛頓宇宙學、宇宙的動力膨脹及溫度發展歷史；宇宙背景微波輻射；大霹靂核合成。
  18. Modern astronomers, gazing at stars and galaxies far away from the earth, can reconstruct what occurred only minutes after the creation of the universe, billions of years ago.

    現代天文學家凝望著遠離地球的星體，星系，從而領悟出數十億年之前宇宙誕生后的短短幾分鐘內發生了哪些現象。
  19. A “ cosmic origins spectrograph ” will examine the structure and composition of the matter concentrated in the “ cosmic web ” ? long, narrow filaments of galaxies and intergalactic gas separated by huge voids

    「宇宙起源光譜儀」將檢查聚集在「宇宙網」 （星系和星系間氣體被巨大的空間分隔所組成的狹長線）中的物質的結構和組成。
  20. Surprisingly, the results indicate that most of the energy released by the infalling gas goes, not into an outpouring of light as is observed in many active galactic nuclei, but into jets of high - energy particles

    令人吃驚的是，結果表明，與大多數活動星系核不同，下落氣體釋放的大部分能量並沒有作為光輻射傾瀉而出，卻是注入到了高能粒子噴流中。
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