Home | Contact | Sitemap | 中文 | CAS
About Us Research People International Cooperation News Education & Training Join Us Journals Papers Resources Links
Location: Home > News > Events
  • Events
  • Seminars
  • Research Trends
  • Discovery points to origin of mysterious ultraviolet radiation
    Author: Update time: 2020-03-11

    Billions of lightyears away, gigantic clouds of hydrogen gas produce a special kind of radiation, a type of ultraviolet light known as Lyman-alpha emissions. The enormous cloudsemitting the light are Lyman-alpha blobs (LABs). LABs are several times larger than our Milky Way galaxy, yet were only discovered 20 years ago. An extremely powerful energy source is necessary to produce this radiation--think the energy output equivalent of billions of our sun--but scientists debate what that energy source could be.

    A new study that published on March 9 in Nature Astronomy provides evidence that the energy sourceis at the center of star-forming galaxies, around which the LABs exist.

    The study focuses on Lyman-alpha blob 6 (LAB-6), whose light was emitted 10.7 billion years ago. It is currently located more than 18.5 billion light years away in the direction of constellation Grus, farther than the distance traveled by light because of the expansion of the universe.The collaborative team led by Yiping Ao of Purple Mountain Observatory discovered a unique feature of LAB-6--its hydrogen gas appeared to fall inwards on itself. LAB-6 is the first LAB with strong evidence of this so-called infalling gas signature.The infalling gas was low in abundance of metallic elements, suggesting that the LAB's infalling hydrogen gas originated in the intergalactic medium, rather than from the star-forming galaxy itself.

    The authors used the Very Large Telescope (VLT) at the European Southern Observatory (ESO) and the Atacama Large Millimeter/Submillimeter Array (ALMA) to obtain the data. The ALMA data can pin down the systemic velocity of the galaxy, and then the optical telescope VLT gives us important spectral light profile of Lyman-alpha emission.

    The authors used the ALMA observation to locate the expected wavelength of the Lyman-alpha emission from the Earth's prospective, if there were no bouncing effect for the Lyman-alpha photons. With the VLT observation, they found that Lyman-alpha emission from this blob shifts into shorter wavelength, implying gas inflow. They used models to analyze the spectrum data and study the kinematics of hydrogen gas.

    LABs are associated with gigantic galaxies that are forming stars at a rate of hundreds to thousands of solar masses per year. Giant halos of Lyman-alpha emissions surround these galaxies, forming the Lyman-alpha gas blobs hundreds of thousands of light years across with power equivalent of about 10 billionsuns. The movement within the gas blobs can tell you something about the state of the galaxy.

    Infalling gas can originate several different ways. It could be the second stage of a galactic fountain--if massive stars die, they explode and push gas outward, which laterfalls inwards. Another option is a cold stream--there are filaments of hydrogen floating between celestial objects that can be pulled into the center of potential well, creating the infalling gas feature.

    The authors' model suggests that the infalling gas in this LAB comes from the latter scenario due to low metallicity confirmed by the model fitting. Additionally, their model indicates that the surrounding gas only produces the energy power equivalent of two solar masses per year, much too low for the amount for the observed Lyman-alpha emission. The findings provide strong evidence thatthe star-forming galaxy is the major contributorof the Lyman-alpha emission, while the infalling gas acts to shape its spectral profile.

    This press release is originally on https://attheu.utah.edu/facultystaff/mysterious-ultraviolet-radiation/.

    The paper is available online via https://www.nature.com/articles/s41550-020-1033-3.

    Original author of this press release:
    Lisa Potter, science writer, University of Utah Communications Office, 801-585-3093,

    Revised by Yiping Ao, research fellow, Purple Mountain Observatory, Chinese Academy of Sciences, ypao@pmo.ac.cn

    Credit: Yiping Ao/VLT/Blanco
    Caption: Three-color image of the sky around Lyman-alpha blob 6 (LAB-6). In green is the Lyman-alpha emission from LAB-6. LAB-6 is 18.5 billion light years away from us in the direction of constellation Grus, with an extension about half million light years. The physical size of the yellow box is 3.26 million light years. Most galaxies seen in this image are foreground galaxies. (Blue: VLT/Hawk-I J band at 1.258 micron; Red: VLT/Hawk-I Ks band at 2.146 micron; Green: Lyman-alpha emission at 0.411 micron with Blanco 4m telescope at the Cerro Tololo Inter-American Observatory)

    Credit: Zheng Zheng
    Caption: A Lyman-alpha emission is of the wavelength represented here as Lyman-alpha line. When gas is outflowing, the Lyman-alpha emission shifts into the longer, redder wavelength. The opposite occurs when gas is inflowing--the Lyman-alpha emission's wavelength appears to get shorter, shifting it into a bluer spectrum.

    Print Text Size: A A A   Close
    Copyright? Purple Mountain Observatory, CAS, No.10 Yuanhua Road, Qixia District, Nanjing 210023, China
    Phone: 0086 25 8333 2000 Fax: 8333 2091 http://english.pmo.cas.cn