This
view, captured by the NASA/ESA Hubble Space Telescope, shows a nearby
spiral galaxy known as NGC 1433. At about 32 million light-years from
Earth, it is a type of very active galaxy known as a Seyfert galaxy — a
classification that accounts for 10% of all galaxies. They have very
bright, luminous centers that are comparable in brightness to that of
our entire galaxy, the Milky Way.
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Galaxy cores are of great interest to astronomers. The centers of
most, if not all, galaxies are thought to contain a supermassive black
hole, surrounded by a disk of in-falling material.
NGC 1433 is being studied as part of a survey of 50 nearby
galaxies known as the Legacy ExtraGalactic UV Survey (LEGUS).
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Ultraviolet radiation is observed from galaxies, mainly tracing the most
recently formed stars. In Seyfert galaxies, ultraviolet light is also
thought to emanate from the accretion discs around their central black
holes. Studying these galaxies in the ultraviolet part of the spectrum
is incredibly useful to study how the gas is behaving near the black
hole. This image was obtained using a mix of ultraviolet, visible, and
infrared light.
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LEGUS will study a full range of properties from a sample of
galaxies, including their internal structure. This Hubble survey will
provide a unique foundation for future observations with the James Webb
Space Telescope (JWST) and the Atacama Large Millimeter/submillimeter
Array (ALMA).
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ALMA has already caught unexpected results relating to the
center of NGC 1433, finding a surprising spiral structure in the
molecular gas close to the center of NGC 1433. The astronomers also
found a jet of material flowing away from the black hole, extending for
only 150 light-years — the smallest such molecular outflow ever observed
in a galaxy beyond our own.
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European Space Agency
Credit: ESA/Hubble & NASA, Acknowledgements: D. Calzetti (UMass) and the LEGUS Team
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