中子星吸積 的英文怎麼說

中文拼音 [zhōngzixīngxījī]
中子星吸積 英文
accretion by neutron star
  • 子 : 子Ⅰ名詞1 （兒子） son 2 （人的通稱） person 3 （古代特指有學問的男人） ancient title of respect f...
  • 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...
  • 吸 : 動詞1 （把液體、氣體等引入體內） inhale; breathe in; draw 2 （吸收） absorb; suck up 3 （吸引） a...
  • 積 : Ⅰ動詞（積累） amass; store up; accumulate Ⅱ形容詞（長時間積累下來的） long standing; long pending...
  1. The model comprising accretion onto a neutron star or black hole companion must still be considered a favored hypothesis.

    在中子星或黑洞伴星上發生吸積的模型，仍應看成是一個有價值的假說。
  2. The temperature range of quasisoft x - ray sources falls just right for an accreting black hole that is more massive than a stellar - mass black hole. however, we should be cautioned that in principle, the low temperatures of many quasisoft x - ray sources can be explained by stellar - mass black holes, neutron stars, and even white dwarfs under very specific physical conditions

    就以類軟射線源的溫度范圍來說，雖然它完全符合那些比恆星型黑洞更大的吸積黑洞，但有一點不能忽略，就是這個溫度在理論上也可以是由恆星型黑洞中子星甚至白矮星在一些特殊物理情況下產生。
  3. In the accretion disks in binary systems or at the centers of galaxies, particle collisions would produce an inflow of mass that is too small by many orders of magnitude to produce the brilliant luminosity of these disks

    在雙星系統或星系中心的吸積盤中，粒子的碰撞只會引起很少的質量向內流動，距離要產生可達到這些圓盤的耀眼亮度，還差了許多個數量級。
  4. Because of the connection between outflow and accretion seen in low - mass stars, surveys of molecular outflows in high - mass ysos can shed light on this debate

    因為在低質量恆星形成中外流與吸積相聯系，在大質量恆星形成區搜尋分子外流將有助於解決這種爭論。
  5. For neutron stars and black holes, accretion disk will emit high - energy x - rays when matters are spiraling in the compact objects, since immense gravitational force can cause substantial heat up of the matters

    對于中子星和黑洞來說，大的重力使吸積盤內物質的溫度大幅上升，發出能量很高的x射線。
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