Publication type: Refereed

  • Publication
    The Hα Galaxy Survey. VIII. Close Companions and Interactions, and the Definition of Starbursts
    We consider the massive star formation properties, radial profiles, and atomic gas masses of those galaxies in our Hα Galaxy Survey that have close companion...
  • Publication
    The IAC Stripe 82 Legacy Project: a wide-area survey for faint surface brightness astronomy
    We present new deep co-adds of data taken within Stripe 82 of the Sloan Digital Sky Survey (SDSS), especially stacked to reach the faintest surface brightness...
  • Publication
    The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars
    Context. The term macroturbulent broadening is commonly used to refer to a certain type of non-rotational broadening affecting the spectral line profiles of O-...
  • Publication
    The IACOB project. I. Rotational velocities in northern Galactic O- and early B-type stars revisited. The impact of other sources of line-broadening
    Context. Stellar rotation is an important parameter in the evolution of massive stars. Accurate and reliable measurements of projected rotational velocities in...
  • Publication
    The IACOB project. II. On the scatter of O-dwarf spectral type - effective temperature calibrations
    Context. We are now in an era of large spectroscopic surveys of OB-type stars. Quantitative spectroscopic analysis of these modern datasets is enabling us to...
  • Publication
    The IACOB project. IV. New predictions for high-degree non-radial mode instability domains in massive stars and their connection with macroturbulent broadening
    Context. Asteroseismology is a powerful tool to access the internal structure of stars. Apart from the important impact of theoretical developments, progress in...
  • Publication
    The IACOB project. IX. Building a modern empirical database of Galactic O9 - B9 supergiants: Sample selection, description, and completeness
    Context. Blue supergiants (BSGs) are key objects for studying the intermediate phases of massive star evolution because they are very useful to constrain...
  • Publication
    The IACOB project. V. Spectroscopic parameters of the O-type stars in the modern grid of standards for spectral classification
    Context. The IACOB and OWN surveys are two ambitious, complementary observational projects which have made available a large multi-epoch spectroscopic database...
  • Publication
    The IACOB project. VI. On the elusive detection of massive O-type stars close to the ZAMS
    Context. The apparent lack of massive O-type stars near the zero-age main sequence, or ZAMS (at ages <2 Myr), is a topic that has been widely discussed in the...