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    Illustration of 4U 0614+091, an X-ray binary system

    Date: 21 Jun 2010
    Satellite: XMM-Newton
    Depicts: Illustration of the X-ray binary system, 4U 0614+091
    Copyright: ESA

    This illustration depicts 4U 0614+091, an exotic binary system composed of two stellar remnants, a neutron star and a white dwarf.

    A long-sought-after emission line of oxygen, carrying the imprint of strong gravitational fields, has been discovered in the XMM-Newton spectrum of this system.

    Astronomers can use this line to probe extreme gravity effects in the region close to the surface of a neutron star.


    Last Update: 21 Jun 2010

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=47230
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    • Image Hi-Res Versions
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    • Related Images
    • Illustration of 4U 0614+091 (annotated)
    • Spectrum of 4U 0614+091
    • See also
    • XMM-Newton line detection provides new tool to probe extreme gravity
    • Related Publications
    • Madej, O.K. et al. [2010]

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