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The rapid formation of a large rotating disk galaxy three billion years after the Big Bang

Author

Listed:
  • R. Genzel

    (Max-Planck-Institut für extraterrestrische Physik (MPE)
    Le Conte Hall, University of California)

  • L. J. Tacconi

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • F. Eisenhauer

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • N. M. Förster Schreiber

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • A. Cimatti

    (Max-Planck-Institut für extraterrestrische Physik (MPE)
    Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri)

  • E. Daddi

    (National Optical Astronomy Observatory)

  • N. Bouché

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • R. Davies

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • M. D. Lehnert

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • D. Lutz

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • N. Nesvadba

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • A. Verma

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • R. Abuter

    (Max-Planck-Institut für extraterrestrische Physik (MPE))

  • K. Shapiro

    (University of California)

  • A. Sternberg

    (Tel Aviv University)

  • A. Renzini

    (Osservatorio Astronomico di Padova)

  • X. Kong

    (University of Science and Technology of China)

  • N. Arimoto

    (National Astronomical Observatory)

  • M. Mignoli

    (Osservatorio Astronomico di Bologna)

Abstract

An epoch-making galaxy Large ground-based telescopes equipped with the latest near-infrared imaging spectroscopes and adaptive optics are capable of observing events that took place at a crucial period of galaxy formation, about 3 billion years after the Big Bang, when the Universe was only about 20% of its present age. Observations of a high-redshift (z=2.38) star-forming galaxy from this epoch reveal its internal structure. A massive rotating protodisk is channelling gas towards an accreting black hole in a central stellar bulge. Previously the timescales and processes involved in the hierarchical build-up of galaxies were matters of conjecture; now they are the stuff of observation.

Suggested Citation

  • R. Genzel & L. J. Tacconi & F. Eisenhauer & N. M. Förster Schreiber & A. Cimatti & E. Daddi & N. Bouché & R. Davies & M. D. Lehnert & D. Lutz & N. Nesvadba & A. Verma & R. Abuter & K. Shapiro & A. Ste, 2006. "The rapid formation of a large rotating disk galaxy three billion years after the Big Bang," Nature, Nature, vol. 442(7104), pages 786-789, August.
  • Handle: RePEc:nat:nature:v:442:y:2006:i:7104:d:10.1038_nature05052
    DOI: 10.1038/nature05052
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