Publication type: Non-refereed

  • Publication
    RXTE observations strengthen the similarities between the black hole candidates IGR J17091-3624 and GRS 1915+105.
    We report on the RXTE follow up observations of the black hole candidate IGR J17091-3624 (ATEL #3144, #3159, #3167, #3203) after the report of mHz quasi...
  • Publication
    S 1988A in M58: Evidence for a High Luminosity at Very Late Times
    Not Available
  • Publication
    S im ulation And Analysis Of VIM Measurements: Feedback On Design Parameters
    The Visible-light Imager and Magnetograph (VIM) proposed for the ESA Solar Orbiter mission will observe a photo spheric spectral line at high spatial resolution...
  • Publication
    S imulations Of Science Data Of The Solo-VIM Instrument
    The SolO-VIM instrument will be a two-dimensional full-Stokes spectro-polarimeter which will provide diffraction-limited vector-magnetograms, Dopplergrams, and...
  • Publication
    S pace Qualification Of A Thin Wafer Lithium Niobate Etalon For The Visible Light Imager And Magnetograph (Vim)
    For the Visible Light Imager and Magnetograph (VIM) a high-resolution filtergraph is under design. The system takes advantage of a lithium niobate (LiNbO3)...
  • Publication
    s-process enrichment in the planetary nebula NGC 3918
    We present deep, high-resolution (R˜40000) UVES at VLT spectrophotometric data of the planetary nebula NGC 3918. This is one of the deepest spectra ever taken...
  • Publication
    s-process enrichment in the planetary nebula NGC 3918. Results from deep echelle spectrophotometry
    Approximately half of the elements with atomic number Z > 30 are created by slow neutron-capture process in the stellar interior of low- and intermediate- mass...
  • Publication
    S-process nucleosynthesis in AGB models with the FST prescription for convection
    The chemical evolution of asymptotic giant branch (AGB) stars depends greatly on the input physics (e.g., mass loss recipe, convective model). Variations in the...
  • Publication
    S-process nucleosynthesis in AGB stars with the full spectrum of turbulence scheme for convection.
    The chemical evolution of asymptotic giant branch (AGB) stars models depends greatly on the input physics (e.g. convective model, mass loss recipe). Variations...