Astrofísicas: Técnicas

  • Publicación
    Near-infrared emission lines trace the state-independent accretion disc wind of the black hole transient MAXI J1820+070
    The black hole transient MAXI J1820+070 displayed optical P Cyg profiles and other wind-related emission line features during the hard state of its discovery...
  • Publicación
    Near-infrared polarimetric adaptive optics observations of NGC 1068: a torus created by a hydromagnetic outflow wind
    We present J' and K' imaging linear polarimetric adaptive optics observations of NGC 1068 using MMT-Pol on the 6.5-m MMT. These observations allow us to study...
  • Publicación
    Near-infrared spectroscopy of 1999 JU3, the target of the Hayabusa 2 mission
    Context. Primitive asteroids contain complex organic material and ices relevant to the origin of life on Earth. These types of asteroids are the target of...
  • Publicación
    Near-infrared study of the stellar population of Sh2-152
    Context. The discovery of new massive star clusters and massive stellar populations in previously known clusters in our Galaxy by means of infrared studies has...
  • Publicación
    Near-term detectability of terrestrial extrasolar planets: TEP network observations of CM Draconis
    Results from a photometric search for extrasolar planetary transits across the eclipsing binary CM Dra are presented. The TEP (Transits of Extrasolar Planets)...
  • Publicación
    Near-ultraviolet absorption distribution of primitive asteroids from spectrophotometric surveys. I. Radial distribution
    Context. Hydrated minerals, such as phyllosilicates, on asteroids can provide constraints on the temperature or compositional distribution of the early Solar...
  • Publicación
    Near-ultraviolet to visible spectroscopy of the Themis and Polana-Eulalia complex families
    Context. Spectrophotometry data of asteroids obtained in the 1980s showed that there are large variations in their near-ultraviolet (NUV) reflectance spectra...
  • Publicación
    Nearby supernova host galaxies from the CALIFA Survey. I. Sample, data analysis, and correlation to star-forming regions
    We use optical integral field spectroscopy (IFS) of nearby supernova (SN) host galaxies (0.005 2.4 Gyr, respectively) than the massive SN Ia hosts (0.04%, 2.01%...
  • Publicación
    New and updated stellar parameters for 71 evolved planet hosts. On the metallicity-giant planet connection<xref ref-type="fn" rid="FN1"><xref ref-type="fn" rid="FN2">⋆<xref ref-type="fn" rid="FN3">⋆⋆
    Context. It is still being debated whether the well-known metallicity-giant planet correlation for dwarf stars is also valid for giant stars. For this reason...