Publication type: Non-refereed

  • Publication
    Widely separated binary systems of very low-mass stars
    In this paper we review some recent detections of wide binary brown dwarf systems and discuss them in the context of the multiplicity properties of very low...
  • Publication
    Will HR8752 become a P Cygni type star?
    As long as the yellow hypergiant HR8752 has been observed spectroscopically it has shown erratic and significant fluctuations in its effective temperature. But...
  • Publication
    Wind Accretion and State Transitions in the Black Hole Binary Cyg X-1
    The black hole binary, Cyg X-1, is generally observed in one of two long duration X-ray states: a low flux, hard spectrum state (most common) and a high flux...
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    Wind Diagnostic from Infrared Lines
    For the large population of massive stars lying behind dust, among which are the youngests and potentially the most massive of our Galaxy, none of the commonly...
  • Publication
    Wind Evaluation Breadboard electronics and software
    WEB, the Wind Evaluation Breadboard, is an Extremely Large Telescope Primary Mirror simulator, developed with the aim of quantifying the ability of a segmented...
  • Publication
    Wind Evaluation Breadboard: mechanical design and analysis, control architecture, dynamic model, and performance simulation
    The Wind Evaluation Breadboard (WEB) for the European Extremely Large Telescope (ELT) is a primary mirror and telescope simulator formed by seven segments...
  • Publication
    Wind tunnel test for the preliminary design of the European Solar Telescope
    The European Solar Telescope (EST) is a 4.2-m solar telescope, based on an aplanatic Gregorian configuration with an alt-azimuthal mount. EST has an open...
  • Publication
    Wind turbulence structure inside telescope enclosures
    Telescope enclosures are used to limit the disturbance caused by the wind on the pointing and tracking performances of telescopes and to preserve primary mirror...
  • Publication
    Winds Driven by Super-Star Clusters
    Here we present a self-consistent stationary solution for spherically symmetric winds driven by massive star clusters under the impact of radiative cooling. We...