Quasars or QSOs类星体或QSOs
Quasars have large red shifts, indicative of great distance from the earth, but have variability with periods of weeks or months which indicate that they are small. Their size is on the order of light weeks, but are brighter than our galaxy which is about 100,000 light years across. The red shift is usually stated in terms of a parameter z which is defined by
![]() 类星体具有大的红移,这表明它们距离地球很远,但它们的变异性具有数周或数月的周期,这表明它们的尺寸很小。它们的尺寸大约为光周,但它们的亮度比我们的银河系大,而银河系的直径大约为100,000光年。红移通常以参数z来表示,其定义为,并且对于超过100个观测到的类星体,z的范围是0.16到3.53。计算v/c得到
The name "quasar" is derived from an early description "QUAsi-StellAR-Objects" .This description was used since they appeared to be faint stars, but they had the dramatically large red shifts which indicated that they were something else. ‘类星体’这个名称来源于早期的一种描述‘QUA si- S tell AR -Objects’。这种描述是在它们看起来像暗淡的恒星时使用的,但它们具有显著的红移,表明它们是某种其他天体。
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More on Quasars关于类星体的更多内容
The observed quasar red shifts correspond to a speed range of .15 c to 0.91 c. Using a Hubble constant of 55 km/s per megaparsec gives distances of 2.6 to 16 billion light years for these quasars. 观测到的类星体红移对应于速度范围为0.15c到0.91c。使用哈勃常数55 km/s每兆秒差距,这些类星体的距离为2.6到16十亿光年。
The evidence on quasars suggests greater luminosity than our entire galaxy of 200 billion stars. The turbulent velocities in the quasars are up to a few 10s of thousands of m/s, so are constantly occurring explosions, i.e., that kind of turbulent velocity in a chemical reaction would make a potent bomb. Some of the quasars are a few light-days across, as evidenced by their periods of variability, and yet much brighter than our entire galaxy which is 100,000 light years across. This makes them about solar system size. The suggested energy source is a black hole with several billion solar masses. 关于类星体的证据表明,其亮度远超过我们整个由2000亿颗恒星组成的星系。类星体中的湍流速度可达几千米每秒,因此经常发生爆炸,即这种湍流速度在化学反应中会形成一种威力巨大的炸弹。一些类星体的直径只有几光日,这从它们的变异性可以得到证实,而它们的亮度却远超过我们整个直径为10万光年的星系。这使它们的尺寸大约与太阳系相当。所提出的能量来源是一种质量达数十亿倍太阳质量的黑洞。
There are examples of multiple images of quasars caused by gravitational lens effects. 有由引力透镜效应引起的类星体多重像的例子。
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Gravitational Lens引力透镜
![]() "In this photograph, light from the distant galaxy bends as it passes through the cluster, dividing the galaxy into five separate images. One image is near the center of the photograph; the others are at 6, 7, 8, and 2 o'clock. The light also has distorted the galaxy's image from a normal spiral shape into a more arc-shaped object. Astronomers are certain the blue-shaped objects are copies of the same galaxy because the shapes are similar. The cluster is 5 billion light-years away in the constellation Pisces, and the blue-shaped galaxy is about 2 times farther away." When the amount of bending is analyzed, the required bending mass is greater than can be accounted for from the visible mass of the cluster, so this is another piece of evidence for the existence of dark matter. 在这张照片中,来自遥远星系的光在穿过星团时发生弯曲,将星系分成五个独立的图像。其中一个图像位于照片的中心;其他四个分别位于6点、7点、8点和2点方向。光也使星系的图像从正常的螺旋形状扭曲成一个更弧形的物体。天文学家确定蓝色形状的物体是同一星系的复制品,因为这些形状相似。星团位于仙女座星座,距离地球50亿光年,而蓝色形状的星系则大约远2倍。当弯曲程度被分析时,所需的弯曲质量大于可以由星团可见物质所解释的量,因此这也是暗物质存在的又一证据。
"Though the gravitational light-bending process is not new, Hubble's high resolution image reveals structures within the blue-shaped galaxy that astronomers have never seen before. Some of the structures are as small as 300 light-years across. The bits of white imbedded in the blue galaxy represent young stars; the dark core inside the ring is dust, the material used to make stars. This information, together with the blue color and unusual "lumpy" appearance, suggests a young, star-making galaxy." 尽管引力透镜效应并不是新现象,但哈勃高分辨率图像揭示了蓝形星系内部一些前所未见的结构。其中一些结构的尺寸仅有300光年。嵌入在蓝形星系中的白色斑点代表年轻恒星;环状结构内部的暗核心是尘埃,是制造恒星的材料。这些信息,加上蓝色色调和不规则的外观,表明这是一个正在形成恒星的年轻星系。
"The picture was taken October 14, 1994 with the Wide Field Planetary Camera-2. Separate exposures in blue and red wavelengths were taken to construct this color picture. Credit: W.N. Colley and E. Turner (Princeton University), J.A. Tyson (Bell Labs, Lucent Technologies) and NASA. " 这张照片于1994年10月14日使用宽场行星照相机-2拍摄。为了构造这张彩色照片,分别拍摄了蓝光和红光的曝光。版权:W.N. Colley和E. Turner(普林斯顿大学),J.A. Tyson(贝尔实验室,Lucent技术)和NASA。
Gravitational lensing has now been observed with a number of galaxies. In a study reported in the Astrophysical Journal in February 2006, Adam Bolton and colleagues at the Harvard-Smithsonian Center for Astrophysics described 19 galaxies that were distorting the images of more distant galaxies that were closely aligned with them. Eight of them were so closely aligned that they bent the light of the more distant galaxy into a ring of light called an Einstein ring. The observations were made by the Hubble Space Telescope, guided toward likely candidates for gravitational lensing by the Sloan Digital Sky Survey. 引力透镜现象现在已经通过多个星系得到了观测。在2006年2月《天体物理学杂志》上的一项研究中,哈佛-史密松天体物理中心的Adam Bolton及其同事描述了19个星系,这些星系使更遥远的星系图像发生了扭曲,这些更遥远的星系与它们有紧密的对齐。其中8个星系对齐得如此紧密,以至于它们将更遥远星系的光弯曲成一个称为爱因斯坦环的光环。这些观测是通过哈勃太空望远镜进行的,该望远镜根据Sloan数字天空调查的可能候选者进行引导。
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