• Mini-jet found near Milky Way's supermas

    From ScienceDaily@1:317/3 to All on Thu Dec 9 21:30:46 2021
    Mini-jet found near Milky Way's supermassive black hole

    Date:
    December 9, 2021
    Source:
    NASA/Goddard Space Flight Center
    Summary:
    Our Milky Way's central black hole has a leak. This supermassive
    black hole looks like it still has the vestiges of a blowtorch-like
    jet dating back several thousand years. NASA's Hubble Space
    Telescope hasn't photographed the phantom jet but has helped find
    circumstantial evidence that it is still pushing feebly into a
    huge hydrogen cloud and then splattering, like the narrow stream
    from a hose aimed into a pile of sand.



    FULL STORY ==========================================================================
    Our Milky Way's central black hole has a leak. This supermassive
    black hole looks like it still has the vestiges of a blowtorch-like jet
    dating back several thousand years. NASA's Hubble Space Telescope hasn't photographed the phantom jet but has helped find circumstantial evidence
    that it is still pushing feebly into a huge hydrogen cloud and then splattering, like the narrow stream from a hose aimed into a pile of sand.


    ==========================================================================
    This is further evidence that the black hole, with a mass of 4.1 million
    Suns, is not a sleeping monster but periodically hiccups as stars and
    gas clouds fall into it. Black holes draw some material into a swirling, orbiting accretion disk where some of the infalling material is swept up
    into outflowing jets that are collimated by the black hole's powerful
    magnetic fields. The narrow "searchlight beams" are accompanied by a
    flood of deadly ionizing radiation.

    "The central black hole is dynamically variable and is currently powered
    down," said Gerald Cecil of the University of North Carolina in Chapel
    Hill. Cecil pieced together, like a jigsaw puzzle, multiwavelength
    observations from a variety of telescopes that suggest the black hole
    burps out mini-jets every time it swallows something hefty, like a gas
    cloud. His multinational team's research has just been published in the Astrophysical Journal.

    In 2013 evidence for a stubby southern jet near the black hole came
    from X-rays detected by NASA's Chandra X-ray Observatory and radio
    waves detected by the Jansky Very Large Array telescope in Socorro, New
    Mexico. This jet too appears to be plowing into gas near the black hole.

    Cecil was curious if there was a northern counter-jet as well. He first
    looked at archival spectra of such molecules as methyl alcohol and
    carbon monosulfide from the ALMA Observatory in Chile (Atacama Large Millimeter/Submillimeter Array), which uses millimeter wavelengths to
    peer through the veils of dust between us and the galactic core. ALMA
    reveals an expanding, narrow linear feature in molecular gas that can
    be traced back at least 15 light-years to the black hole.

    By connecting the dots, Cecil next found in Hubble infrared-wavelength
    images a glowing, inflating bubble of hot gas that aligns to the jet at a distance of at least 35 light-years from the black hole. His team suggests
    that the black hole jet has plowed into it, inflating the bubble. These
    two residual effects of the fading jet are the only visual evidence of
    it impacting molecular gas.



    ==========================================================================
    As it blows through the gas the jet hits material and bends along multiple streams. "The streams percolate out of the Milky Way's dense gas disk,"
    said co-author Alex Wagner of Tsukuba University in Japan. "The jet
    diverges from a pencil beam into tendrils, like that of an octopus." This outflow creates a series of expanding bubbles that extend out to at least
    500 light-years. This larger "soap bubble" structure has been mapped at
    various wavelengths by other telescopes.

    Wagner and Cecil next ran supercomputer models of jet outflows in a
    simulated Milky Way disk, which reproduced the observations. "Like in archeology, you dig and dig to find older and older artifacts until
    you come upon remnants of a grand civilization," said Cecil. Wagner's conclusion: "Our central black hole clearly surged in luminosity at
    least 1 millionfold in the last million years.

    That sufficed for a jet to punch into the Galactic halo." Previous observations by Hubble and other telescopes found evidence that the Milky
    Way's black hole had an outburst about 2-4 million years ago. That was energetic enough to create an immense pair of bubbles towering above our
    galaxy that glow in gamma-rays. They were first discovered by NASA's
    Fermi Gamma-ray Space Telescope in 2010 and are surrounded by X-ray
    bubbles that were discovered in 2003 by the ROSAT satellite and mapped
    fully in 2020 by the eROSITA satellite.

    Hubble ultraviolet-light spectra have been used to measure the expansion velocity and composition of the ballooning lobes. Hubble spectra later
    found that the burst was so powerful that it lit up a gaseous structure,
    called the Magellanic stream, at about 200,000 light-years from the
    galactic center. Gas is glowing from that event even today.

    To get a better idea of what's going on, Cecil looked at Hubble and
    radio images of another galaxy with a black hole outflow. Located 47
    million light- years away, the active spiral galaxy NGC 1068 has a
    string of bubble features aligned along an outflow from the very active
    black hole at its center. Cecil found that the scales of the radio and
    X-ray structures emerging from both NGC 1068 and our Milky Way are very similar. "A bow shock bubble at the top of the NGC 1068 outflow coincides
    with the scale of the Fermi bubble start in the Milky Way. NGC 1068 may
    be showing us what the Milky Way was doing during its major power surge
    several million years ago." The residual jet feature is close enough
    to the Milky Way's black hole that it would become much more prominent
    only a few decades after the black hole powers up again. Cecil notes that
    "the black hole need only increase its luminosity by a hundredfold over
    that time to refill the jet channel with emitting particles.

    It would be cool to see how far the jet gets in that outburst. To reach
    into the Fermi gamma-ray bubbles would require that the jet sustain for hundreds of thousands of years because those bubbles are each 50,000
    light years across!" The anticipated images of the black hole's shadow
    made with the National Science Foundation's Event Horizon Telescope may
    reveal where and how the jet is launched.

    Video of mini jet near the Milky Way's supermassive black
    hole: https:// www.youtube.com/watch?v=zxqQ4G0NOhI&t=144s ========================================================================== Story Source: Materials provided by
    NASA/Goddard_Space_Flight_Center. Note: Content may be edited for style
    and length.


    ========================================================================== Journal Reference:
    1. Gerald Cecil, Alexander Y. Wagner, Joss Bland-Hawthorn, Geoffrey V.

    Bicknell, Dipanjan Mukherjee. Tracing the Milky Way's Vestigial
    Nuclear Jet. The Astrophysical Journal, 2021; 922 (2): 254 DOI:
    10.3847/1538- 4357/ac224f ==========================================================================

    Link to news story: https://www.sciencedaily.com/releases/2021/12/211209201656.htm

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