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Hubble Confirms First RELHIC, a Starless Dark-Matter Cloud Near M94

Deep imaging paired with radio mapping shows a compact gas cloud held by a low-mass halo at the brink of galaxy formation.

Overview

  • The object, nicknamed Cloud-9, lies about 14 million light-years away on the outskirts of the spiral galaxy Messier 94.
  • First identified by FAST and confirmed by the Green Bank Telescope and the Very Large Array, it was shown by Hubble’s ACS to contain no stars, with injection simulations indicating any faint population would have been seen.
  • Observations find a neutral-hydrogen core roughly 4,900 light-years across with about one million solar masses of gas inside a dark-matter halo estimated at around five billion solar masses.
  • Cloud-9’s compact, nearly spherical morphology and slight gas distortions in high-resolution radio maps suggest a physical association or interaction with M94.
  • The study, led by STScI researchers, is published in The Astrophysical Journal Letters and presented at the AAS meeting, and the team expects deeper surveys to uncover more such failed galaxies.