Astrophysical: Star formation

  • Publication
    Merger-driven star formation activity in Cl J1449+0856 at z = 1.99 as seen by ALMA and JVLA
    We use Atacama Large Millimetre Array and Jansky Very Large Array observations of the galaxy cluster Cl J1449+0856 at z = 1.99, in order to study how dust...
  • Publication
    Metallicity effects on starburst.
    Not Available
  • Publication
    Metallicity profiles of ultradiffuse galaxies in NIHAO simulations
    Supernovae feedback driven expansion has proven to be a viable mechanism to explain the average properties, such as size, colour, mass, and internal kinematics...
  • Publication
    Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the cosmic noon with a SPICA-like mission
    We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering...
  • Talk
    MILES: population synthesis for the 21st century
    We present the new stellar population synthesis models based on the empirical stellar spectral library MILES, which can be regarded nowadays as standard in the...
  • Publication
    Modeling an accretion disk in NGC 985
    An optically thick relativistic Keplerian accretion disk model is used to fit the broad component of the H-alpha, H-beta, and He I 5876 A emission line profiles...
  • Publication
    Modelling the Mg[b] Spectroscopic Index with the Tunable Filters of OSIRIS
    We present our first attempt to model a new metallicity indicator for old and intermediate aged stellar populations on the basis of the Mg[b] absorption index...
  • Publication
    Molecular gas and star formation within 12 strong galactic bars observed with IRAM-30 m
    Context. While some galactic bars show recent massive star formation (SF) along them, some others do not. Whether bars with low level of SF are a consequence of...
  • Talk
    Molecular gas in galaxies, and evolution with redshift
    I will review some recent results about the molecular content of galaxies and its dynamics, obtained from CO lines, dense tracers (HCN,HCO+), or the dust...