• High-speed propeller star is fastest spi

    From ScienceDaily@1337:3/111 to All on Mon Nov 22 21:30:28 2021
    High-speed propeller star is fastest spinning white dwarf

    November 22, 2021
    University of Warwick
    A white dwarf star that completes a full rotation once every 25
    seconds is the fastest spinning confirmed white dwarf, according
    to a team of astronomers.

    FULL STORY ==========================================================================
    A white dwarf star that completes a full rotation once every 25 seconds
    is the fastest spinning confirmed white dwarf, according to a team of astronomers led by the University of Warwick.

    They have established the spin period of the star for the first time, confirming it as an extremely rare example of a magnetic propeller system:
    the white dwarf is pulling gaseous plasma from a nearby companion star
    and flinging it into space at around 3000 kilometres per second.

    Reported today (22 November) in the journal Monthly Notices of the Royal Astronomical Society: Letters, it is only the second magnetic propeller
    white dwarf to have been identified in over seventy years thanks to a combination of powerful and sensitive instruments that allowed scientists
    to catch a glimpse of the speeding star.

    The study was led by the University of Warwick with the University of Sheffield, and funded by the Science and Technology Facilities Council
    (STFC), part of UK Research and Innovation, and the Leverhulme Trust.

    A white dwarf is a star that has burnt up all of its fuel and shed its
    outer layers, now undergoing a process of shrinking and cooling over
    millions of years. The star that the Warwick team observed, named LAMOST J024048.51+195226.9 -- or J0240+1952 for short, is the size of the Earth
    but is thought to be at least 200,000 times more massive. It is part of
    a binary star system and its immense gravity is pulling material from
    its larger companion star in the form of plasma.

    In the past, this plasma was falling onto the white dwarf's equator at
    high speed, providing the energy that has given it this dizzyingly fast
    spin. Put into context, one rotation of the planet Earth takes 24 hours,
    while the equivalent on J0240+1952 is a mere 25 seconds. That's almost 20% faster than the confirmed white dwarf with the most comparable spin rate,
    which completes a rotation in just over 29 seconds.

    ========================================================================== However, at some point in its evolutionary history J0240+1952 developed
    a strong magnetic field. The magnetic field acts a protective barrier,
    causing most of the falling plasma to be propelled away from the white
    dwarf. The remainder will flow towards the star's magnetic poles. It
    gathers in bright spots on the surface of the star and as these rotate in
    and out of view they cause pulsations in the light that the astronomers
    observe from Earth, which they then used to measure the rotation of the
    entire star.

    Lead author Dr Ingrid Pelisoli of the University of Warwick Department
    of Physics said: "J0240+1952 will have completed several rotations in
    the short amount of time that people take to read about it, it is really incredible. The rotation is so fast that the white dwarf must have an
    above average mass just to stay together and not be torn apart.

    "It is pulling material from its companion star due to its gravitational effect, but as that gets closer to the white dwarf the magnetic field
    starts to dominate. This type of gas is highly conducting and picks up a
    lot of speed from this process, which propels it away from the star and
    out into space." J0240+1952 is one of only two stars with this magnetic propeller system discovered in over past seventy years. Although material
    being flung out of the star was first observed in 2020, astronomers had
    not been able to confirm the presence of a rapid spin that is a main
    ingredient of a magnetic propeller, as the pulsations are too fast and
    dim for other telescopes to observe.

    To visualise the star at that speed for the first time, the University
    of Warwick team used the highly sensitive HiPERCAM instrument, jointly
    operated by Warwick and the University of Sheffield with funding from
    the European Research Council. This was specially mounted on the largest functioning optical telescope in the world, the 10 metre diameter Gran Telescopio Canarias in La Palma, to capture as much light as possible.

    "These kinds of studies are possible thanks to the unique combination
    of the fast imaging capability of HiPERCAM with the largest collecting
    area in the world provided by GTC," said Antonio Cabrera, Head of GTC
    Science Operations.

    Co-author Professor Tom Marsh from the University of Warwick Department
    of Physics adds: "It's only the second time that we have found one
    of these magnetic propeller systems, so we now know it's not a unique occurrence. It establishes that the magnetic propeller mechanism is a
    generic property that operates in these binaries, if the circumstances
    are right.

    "The second discovery is almost as important as the first as
    you develop a model for the first and with the second you can
    test it to see if that model works. This latest discovery
    has shown that the model works really well, it predicted
    that the star had to be spinning fast, and indeed it does." ========================================================================== Story Source: Materials provided by University_of_Warwick. Note: Content
    may be edited for style and length.

    ========================================================================== Journal Reference:
    1. Ingrid Pelisoli, T R Marsh, V S Dhillon, E Breedt, A J Brown,
    M J Dyer, M
    J Green, P Kerry, S P Littlefair, S G Parsons, D I Sahman, J F Wild.

    Found: a rapidly spinning white dwarf in LAMOST J024048.51 195226.9.

    Monthly Notices of the Royal Astronomical Society: Letters,
    Volume 509, Issue 1, January 2022, Pages L31%u2013L36 DOI:
    10.1093/mnrasl/slab116 ==========================================================================

    Link to news story: https://www.sciencedaily.com/releases/2021/11/211122135446.htm

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