蜜臀av性久久久久|国产免费久久精品99|国产99久久久久久免费|成人精品一区二区三区在线|日韩精品一区二区av在线|国产亚洲欧美在线观看四区|色噜噜综合亚洲av中文无码|99久久久国产精品免费播放器

<cite id="ygcks"><center id="ygcks"></center></cite>
  • 
    
  • <rt id="ygcks"></rt>
    <cite id="ygcks"></cite>
  • <li id="ygcks"><source id="ygcks"></source></li> <button id="ygcks"></button>
  • <button id="ygcks"></button>
    <button id="ygcks"><input id="ygcks"></input></button>
    
    
    <abbr id="ygcks"><source id="ygcks"></source></abbr>
    
    
    
     
    
    

    Astronomers see how black hole rips apart star

    Source: Xinhua| 2018-06-15 03:38:36|Editor: Chengcheng
    Video PlayerClose

    WASHINGTON, June 14 (Xinhua) -- Astronomers have directly "seen" the formation and expansion of a fast-moving jet of material ejected when the powerful gravity of a supermassive black hole ripped apart a star that wandered too close to it.

    They reported on Thursday in the journal Science the event in a pair of colliding galaxies called Arp 299, nearly 150 million light-years from Earth.

    At the core of one of the galaxies, a black hole 20 million times more massive than the Sun shredded a star more than twice the Sun's mass, setting off a chain of events that revealed important details of the violent encounter, according to the study.

    Theorists suggested that material pulled from the doomed star forms a rotating disk around the black hole, emitting intense X-rays and visible light, and also launches jets of material outward from the poles of the disk at nearly the speed of light.

    "Never before have we been able to directly observe the formation and evolution of a jet from one of these events," said Miguel Perez-Torres with the Astrophysical Institute of Andalusia in Granada, Spain.

    The first indication came on Jan. 30, 2005, when astronomers using the William Herschel Telescope in the Canary Islands discovered a bright burst of infrared emission coming from the nucleus of one of the colliding galaxies in Arp 299.

    On July 17, 2005, the Very Long Baseline Array (VLBA) in the United States revealed a new, distinct source of radio emission from the same location.

    "As time passed, the new object stayed bright at infrared and radio wavelengths, but not in visible light and X-rays," said Seppo Mattila with the University of Turku in Finland.

    "The most likely explanation is that thick interstellar gas and dust near the galaxy's center absorbed the X-rays and visible light, then re-radiated it as infrared," said Mattila.

    Also, continued observations with the VLBA, the European VLBI Network (EVN), and other radio telescopes, carried out over nearly a decade, showed the source of radio emission expanding in one direction, just as expected for a jet.

    The measured expansion indicated that the material in the jet moved at an average of one-fourth the speed of light. The radio waves are not absorbed in the core of the galaxy, but find their way through it to reach the Earth.

    The discovery, the scientists said, came as a surprise. The initial infrared burst was discovered as part of a project that sought to detect supernova explosions in such colliding pairs of galaxies. Arp 299 has seen numerous stellar explosions, and has been dubbed a "supernova factory."

    This new object originally was considered to be a supernova explosion. Only in 2011, six years after discovery, the radio-emitting portion began to show an elongation.

    Subsequent monitoring showed the expansion growing, confirming that what the scientists are seeing is a jet, not a supernova.

    TOP STORIES
    EDITOR’S CHOICE
    MOST VIEWED
    EXPLORE XINHUANET
    010020070750000000000000011100001372544201
    永仁县| 阿城市| 车致| 神池县| 上杭县| 惠州市| 昭苏县| 清河县| 洮南市| 同心县| 含山县| 宿州市| 盐边县| 壤塘县| 百色市| 通城县| 虹口区| 兰州市| 吉林省| 长乐市| 札达县| 迁西县| 沭阳县| 孝昌县| 洛浦县| 桃江县| 六安市| 灌南县| 方山县| 惠安县| 怀仁县| 临澧县| 康保县| 嘉善县| 靖边县| 方城县| 龙南县| 富锦市| 阜平县| 包头市| 武山县|