Astrophysical: Star formation

  • Publication
    The EDGE-CALIFA Survey: An integral field unit-based integrated molecular gas database for galaxy evolution studies in the Local Universe
    Studying galaxy evolution requires knowledge not only of the stellar properties, but also of the interstellar medium (in particular the molecular phase) out of...
  • Publication
    The EDGE-CALIFA survey: exploring the role of molecular gas on galaxy star formation quenching
    Understanding how galaxies cease to form stars represents an outstanding challenge for galaxy evolution theories. This process of "star formation quenching" has...
  • Publication
    The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
    Galaxy evolution is largely driven by star formation activity or by the cessation of it, also called star formation quenching. In this paper, we present...
  • Publication
    The EDGE-CALIFA survey: The effect of active galactic nucleus feedback on the integrated properties of galaxies at different stages of their evolution
    Galaxy quenching, the intricate process through which galaxies transition from active star-forming states to retired ones, remains a complex phenomenon that...
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    The EDGE-CALIFA survey: the influence of galactic rotation on the molecular depletion time across the Hubble sequence
    We present a kpc-scale analysis of the relationship between the molecular depletion time (τ^mol_dep) and the orbital time (τorb) across the field of 39 face-on...
  • Publication
    The EDGE–CALIFA Survey: Variations in the Molecular Gas Depletion Time in Local Galaxies
    We present results from the EDGE survey, a spatially resolved CO(1‑0) follow-up to CALIFA, an optical Integral Field Unit survey of local galaxies. By combining...
  • Publication
    The effect of environment on star forming galaxies at redshift 1 First insight from PACS (Corrigendum)
    Not Available
  • Publication
    The effect of environment on star forming galaxies at redshift. I. First insight from PACS
    We use deep 70, 100 and 160 μm observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS...
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    The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
    Recent observational and theoretical studies indicate that the stellar initial mass function (IMF) varies systematically with the environment (star formation...