Tipo de publicación: Con árbitro

  • Publicación
    Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagittarii
    Context. The overwhelming majority of cataclysmic variables (CVs) have orbital periods shorter than 10 h. However, a few have much longer orbital periods, and...
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    Revisiting the formation history of the minor-axis dust lane galaxy NGC 1947
    In this paper, we present a detailed study of the peculiar early-type galaxy NGC 1947. The main goal of this work is to constrain the dynamical status and the...
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    Revisiting the fundamental parameters for the black hole X-ray transient Swift J1753.5–0127
    We present time-resolved Gran Telescopio Canarias optical spectroscopy and William Herschel Telescope i-band photometry of the X-ray transient SWIFT J1753.5...
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    Revisiting the globular clusters of NGC 1052-DF2
    The ultra-diffuse galaxy (UDG) NGC 1052-DF2 has captured the interest of astronomers ever since the low velocity dispersion measured from ten globular clusters...
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    Revisiting the Hubble sequence in the SDSS DR7 spectroscopic sample: a publicly available Bayesian automated classification
    We present an automated morphological classification in 4 types (E, S0, Sab, Scd) of ~700 000 galaxies from the SDSS DR7 spectroscopic sample based on support...
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    Revisiting the hypothesis of purely stochastic excitation of global p modes in the Sun
    Context. In solar-like oscillators, acoustic waves are excited by turbulent motion in the convective envelope and propagate inward, generating a variety of...
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    Revisiting the impact of stellar magnetic activity on the detection of solar-like oscillations by Kepler
    Over 2,000 stars were observed for one month with a high enough cadence in order to look for acoustic modes during the survey phase of the Kepler mission. Solar...
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    Revisiting the infrared spectra of active galactic nuclei with a new torus emission model
    We describe improved modelling of the emission by dust in a toroidal-like structure heated by a central illuminating source within active galactic nuclei (AGNs)...
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    Revisiting the Li Abundances of Stars with and without Detected Planets from High-resolution Spectroscopy
    Whether the presence of planets affects the lithium (Li) abundance of their host stars is still an open question. To investigate the difference in the Li...