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Showing 1–9 of 9 results
Advanced filters: Author: E. Daddi Clear advanced filters
  • A massive starburst galaxy at redshift 1.4 is ejecting 46 ± 13% of its molecular gas mass at a rate of ≥ 10,000 M yr−1, owing to a merger rather than feedback processes. The implied statistics suggest that similar events are potentially a major quenching channel.

    • Annagrazia Puglisi
    • Emanuele Daddi
    • Giulia Rodighiero
    Research
    Nature Astronomy
    Volume: 5, P: 319-330
  • A study of 36 massive galaxies at redshifts between 5 and 9 from the JWST FRESCO survey finds that galaxy formation of the most massive galaxies is 2–3 times higher than the most efficient galaxies at later epochs.

    • Mengyuan Xiao
    • Pascal A. Oesch
    • J. Stuart B. Wyithe
    Research
    Nature
    Volume: 635, P: 311-315
  • Deep ALMA archival observations of submillimetre-bright galaxies at high redshifts show that spheroidal bulges formed much earlier than expected and are directly generated by star formation within the cores of highly luminous starburst galaxies.

    • Qing-Hua Tan
    • Emanuele Daddi
    • Francesco Valentino
    Research
    Nature
    Volume: 636, P: 69-74
  • Observations of a luminous star-forming galaxy when the Universe was only 20% of its current age reveal high gas surface densities, large star formation rate and moderately young stellar ages, suggesting rapid assembly, fragmentation and conversion to stars of an initially very gas-rich protodisk.

    • R. Genzel
    • L. J. Tacconi
    • M. Mignoli
    Research
    Nature
    Volume: 442, P: 786-789
  • A sample of quiescent early-type galaxies (ETGs) — home to most of the stars in the local Universe — at z ~ 1.8 contain two orders of magnitude more dust at a fixed stellar mass than local ETGs. This implies a higher gas content, at odds with the idea that star formation at this redshift is quenched by gas removal.

    • R. Gobat
    • E. Daddi
    • F. Valentino
    Research
    Nature Astronomy
    Volume: 2, P: 239-246