Talk format: Breaking News

  • Talk
    Magnetic fields and the outer rotation curve of M31
    Recent observations of the rotation curve of M31 show a rise of the outer part that cannot be understood in terms of standard dark matter models or...
  • Talk
    Metallicities, Age-Metallicity Relationships, and Kinematics of Red Giant Branch Stars in the Outer Disk of the Large Magellanic Cloud
    The outer disk of the Large Magellanic Cloud (LMC) is studied in order to unveil clues about its formation and evolution. We have obtained deep color-magnitude...
  • Talk
    MUSE-AO view of the starburst-AGN connection: NGC 7130
    We present the discovery of a small 0.2'' (60 pc) radius kinematically decoupled core, as well as an outflow jet, in the archetypical AGN-starburst "composite"...
  • Talk
    New insight into the T-type planetary mass population in the Sigma Orionis cluster
    The proper characterization of the least massive population of the young Sigma Orionis star cluster is required to understand the form of the cluster mass...
  • Talk
    On the curvature of dust lanes in galactic bars
    We test the theoretical prediction that the straightest dust lanes in bars are found in strongly barred galaxies, or more specifically, that the degree of...
  • Talk
    On the probable existence of an abrupt magnetization in the upper chromosphere of the quiet Sun
    We report on a detailed radiative transfer modeling of the observed scattering polarization in the H-alpha line, which allows us to infer quantitative...
  • Talk
    Probing gamma-ray production in relativistic jets of flat spectrum radio quasars
    The MAGIC telescopes discovered very high energy (VHE, E>100 GeV) gamma-ray emission coming from the distant Flat Spectrum Radio Quasar (FSRQ) PKS 1222+21 (4C...
  • Talk
    Relationship between Hubble type and spectroscopic class in local galaxies
    We compare the Hubble type and the spectroscopic class of the galaxies with spectra in SDSS/DR7. As it is long known, elliptical galaxies tend to be red whereas...
  • Talk
    Rubidium-rich asymptotic giant branch stars in the Magellanic Clouds
    Asymptotic Giant Branch (AGB) stars are a principal source of gas and dust input into the interstellar medium, being an important driver of chemical evolution...