Publications by authors named "Bjorn H C Emonts"

Our knowledge of galaxy formation and evolution has incredibly progressed through multi-wavelength observational constraints of the interstellar medium (ISM) of galaxies at all cosmic epochs. However, little is known about the physical properties of the more diffuse and lower surface brightness reservoir of gas and dust that extends beyond ISM scales and fills dark matter haloes of galaxies up to their virial radii, the circumgalactic medium (CGM). New theoretical studies increasingly stress the relevance of the latter for understanding the feedback and feeding mechanisms that shape galaxies across cosmic times, whose cumulative effects leave clear imprints into the CGM.

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Article Synopsis
  • The early Universe's galaxy growth is fueled by accretion of gas from surrounding areas.
  • A 100 kiloparsec-long filamentary stream of gas was discovered linking to the massive radio galaxy 4C 41.17.
  • This gas stream has been identified as a key source for star formation, highlighting that materials for new stars can exist in cosmic streams outside galaxies.
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