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Black Holes Are Missing in the Early Universe – But Scientists Are on the Hunt

Upcoming radio telescope sky surveys are set to observe millions of early Universe galaxies. However, to handle this massive influx of data, automatic tools are essential. An algorithm developed by a team from the Institute of Astrophysics and Space Sciences (IA) at the Faculty of Sciences, Universi

Astronomers think they finally know origin of enormous cosmic smoke rings

Astronomers Solve Mystery of Odd Radio Circles

Astronomers Solve Mystery of Odd Radio Circles
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Ionized gas extends over 40 kpc in an odd radio circle host galaxy

A new class of extragalactic astronomical sources discovered in 2021, named odd radio circles (ORCs)1, are large rings of faint, diffuse radio continuum emission spanning approximately 1 arcminute on the sky. Galaxies at the centres of several ORCs have photometric redshifts of z ≃ 0.3–0.6, implying physical scales of several 100 kpc in diameter for the radio emission, the origin of which is unknown. Here we report spectroscopic data on an ORC including strong [O ii] emission tracing ionized gas in the central galaxy of ORC4 at z = 0.4512. The physical extent of the [O ii] emission is approximately 40 kpc in diameter, larger than expected for a typical early-type galaxy2 but an order of magnitude smaller than the large-scale radio continuum emission. We detect an approximately 200 km s−1 velocity gradient across the [O ii] nebula, as well as a high velocity dispersion of approximately 180 km s−1.

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