And that's what powers active galaxies!
这就是活跃星系的动力!
单词 | Active Galaxy |
释义 |
Active Galaxy
原声例句
Crash Course 天文篇 And that's what powers active galaxies! 这就是活跃星系的动力! Crash Course 天文篇 Some, called active galaxies, pour out far more energy than normal ones. 有一些被称为活动星系的星系,它们释放出的能量比正常星系多得多。 Crash Course 天文篇 How could they power active galaxies, the brightest objects in the Universe? ” 它们是如何给活动星系——宇宙中最亮的物体——提供能量的呢?” Crash Course 天文篇 Our black hole is quiescent, that is, not actively feeding, so we're not an active galaxy. 我们的黑洞是静止的,也就是说,我们不是一个活跃的星系。 Crash Course 天文篇 Active galaxies are so bright they can be seen clear across the Universe. 活动星系非常明亮,在整个宇宙中都能清晰地看到它们。 Crash Course 天文篇 Spirals, ellipticals, irregulars, peculiars, active galaxies… in many clusters, a huge elliptical galaxy sits right at the very center. 螺旋星系、椭圆星系、不规则星系、特殊星系、活动星系… … 在许多星系团中,有一个巨大的椭圆星系就位于正中央。 Crash Course 天文篇 Today you learned that active galaxies pour out lots of energy, due to their central supermassive black holes gobbling down matter. 今天你学到了活跃的星系会释放出大量的能量,因为它们中心的超大质量黑洞会吞噬物质。 Crash Course 天文篇 Active galaxies can look pretty different from each other, and we now think that's due to our viewing angle on their accretion disk. 活动星系之间可能看起来非常不同,我们现在认为这是由于我们观察它们吸积盘的角度不同造成的。 Crash Course 天文篇 Astronomers gave them the generic name “active galaxies, ” and classified them into various subcategories depending on how they emitted their light, and what kind of spectra they had. 天文学家将它们命名为“活动星系”,并根据它们发出光的方式和光谱的类型将它们分为不同的子类。
中文百科
活动星系核 Active galactic nucleus(重定向自Active Galaxy)
![]() ![]() ![]() ![]() 活动星系核(Active Galactic Nucleus,缩写为AGN)是一个星系中央区有比普通的星系的强烈很多的光度,至少部分波段或甚至可能全部波段里都发出很强的电磁波谱。被观察到的发射复盖从无线电波,微波,红外线,可见光,紫外线,X射线,到伽玛射线。光度大约在10-10J/s之间。容纳活动星系核的宿主星系为活跃星系。活跃星系核是这些星系明亮的核心部分,尺度通常在1光年上下,只占整个活跃星系的很小一部分。活动星系核(AGN)是在宇宙中的电磁辐射的最明亮的持久性的来源,并且因此可以被用作发现远方天体的方法;其演化的宇宙时间函数也设置了宇宙模型的制约条件。
英语百科
Active galactic nucleus 活动星系核(重定向自Active Galaxy)
![]() ![]() ![]() ![]() An active galactic nucleus (AGN) is a compact region at the center of a galaxy that has a much higher than normal luminosity over at least some portion – and possibly all – of the electromagnetic spectrum. Such excess emission has been observed in the radio, microwaves, infrared, optical, ultra-violet, X-ray and gamma ray wavebands. A galaxy hosting an AGN is called an active galaxy. The radiation from an AGN is believed to be a result of accretion of mass by a supermassive black hole at the center of its host galaxy. AGN are the most luminous persistent sources of electromagnetic radiation in the universe, and as such can be used as a means of discovering distant objects; their evolution as a function of cosmic time also puts constraints on models of the cosmos. |
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