Tipo de publicación: Con árbitro

  • Publicación
    The effective temperature scale of giant stars (F0-K5). II. Empirical calibration of Teff versus colours and [Fe/H]
    We present calibrations of the effective temperatures of giant stars versus [Fe/H] and colours (U-V), (B-V), (R-I), (V-R), (V-I), (V-K), (J-H), (J-K), (I-K), (V...
  • Publicación
    The effective temperature scale of giant stars (F0-K5). III. Stellar radii and the calibration of convection
    We present an analysis of radii of giant stars with 6200 K>= T_eff >= 3800 K based on angular diameters obtained by means of the IRFM and distances computed...
  • Publicación
    The Effective Temperatures of Hot Stars. II. The Early-O Types
    We derived the stellar parameters of a sample of Galactic early-O type stars by analyzing their UV and far-UV spectra from the Far Ultraviolet Spectroscopic...
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    The Effective Temperatures of Mid-O Stars
    We derived photospheric parameters, mass-loss rates, and wind velocities of Galactic O6-O7 stars by analyzing high-resolution spectra in the far-UV and UV...
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    The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
    Feedback from active galactic nuclei (AGNs) has become established as a fundamental process in the evolution of the most massive galaxies. Its impact on Milky...
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    The effects of environment on galaxies' dynamical structures: From simulations to observations
    We studied the effects of cluster environments on galactic structures by using the TNG50 cosmological simulation and observed galaxies in the Fornax cluster. We...
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    The effects of galaxy formation on the matter power spectrum: a challenge for precision cosmology
    Upcoming weak lensing surveys, such as LSST, EUCLID and WFIRST, aim to measure the matter power spectrum with unprecedented accuracy. In order to fully exploit...
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    The Effects of Magnetic-field Geometry on Longitudinal Oscillations of Solar Prominences
    We investigate the influence of the geometry of the solar filament magnetic structure on the large-amplitude longitudinal oscillations. A representative...
  • Publicación
    The effects of magnetic-field geometry on longitudinal oscillations of solar prominences: Cross-sectional area variation for thin tubes
    Context. Solar prominences are subject to both field-aligned (longitudinal) and transverse oscillatory motions, as evidenced by an increasing number of...