• → European Space Agency

      • Space for Europe
      • Space News
      • Space in Images
      • Space in Videos
    • About Us

      • Welcome to ESA
      • DG's News and Views
      • For Member State Delegations
      • Business with ESA
      • ESA Exhibitions
      • ESA Publications
      • Careers at ESA
    • Our Activities

      • Space News
      • Observing the Earth
      • Human Spaceflight
      • Launchers
      • Navigation
      • Space Science
      • Space Engineering
      • Operations
      • Technology
      • Telecommunications & Integrated Applications
    • For Public

    • For Media

    • For Educators

    • For Kids

    • ESA

    • Space in Images

    ESA > Space in Images > 2008 > 04 > Broad Absorption Line quasar

    Free Search (10891 images)

    • Recently Added
    • Advanced Search

    Broad Absorption Line quasar

    (29.05 MB)
    Views: 2
    Rating: 0.00/5 (0 votes cast)

    Rate this Image

    • Currently 0 out of 5 Stars.
    • 1
    • 2
    • 3
    • 4
    • 5

    Thank you for rating!

    You have already rated this page, you can only rate it once!

    Your rating has been changed, thanks for rating!

    Share this Image

    Post to Facebook Post to MySpace Post to Delicious Post to Digg Post to Twitter

    Details

    Open/Close
    • Title Broad Absorption Line quasar
    • Released 04/04/2008 2:19 pm
    • Copyright ESA (Animation by C. Carreau)
    • Description

      Animation of a rare type of quasar, called a broad absorption line (BAL) quasar.

      Quasars are vast cosmic engines that pump energy into their surroundings. It is thought an enormous black hole drives each quasar.

      XMM-Newton has been surprised by a BAL quasar from which it has detected a higher number of X-rays than thought possible. The observation gives new insight into the powerful processes shaping galaxies during their formation and evolution.

      About 10-20% of all quasars are BAL quasars, which get their name from a thick cocoon of gas surrounding the quasar. Most researchers believe that gas flows away from a BAL quasar along the equatorial direction of the accretion disc. These quasars show little X-ray emission, indicating that there is enough gas to absorb most of the X-rays given out from the region near the black hole.

      But as discovered with XMM-Newton, some BAL quasars appear to be spewing material out along their polar axes, at right angles to the accretion discs.


    TAGS

    Open/Close
    • Click on the tags to find the matching images.
    • Activity Space Science
    • Mission XMM-Newton
    • Keywords Astronomy targets

    TAGS

    Open/Close

    Details

    Open/Close

    RELATED IMAGES

    • BAL quasar, top view
      BAL quasar, top view
      Released: 07/04/2008
      Rating
    • BAL quasar, side view
      BAL quasar, side view
      Released: 07/04/2008
      Rating

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Facebook
    • Livestream
    • Subscribe
    • App Store
    • LATEST ARTICLES
    • · Proba-V opens its eyes
    • · First new Galileo satellite arri…
    • · Next destination: space
    • · Leak repaired on International S…
    • · After Chelyabinsk: European expe…
    • FAQ

    • Jobs at ESA

    • Site Map

    • Contacts

    • Terms and conditions