Publication type: Non-refereed

  • Publication
    Hunting Exoplanets with Single-Mode Optical Interferometry
    The GRAVITY instrument was primarily conceived for imaging and astrometry of the Galactic centre. However, its sensitivity and astrometric capabilities have...
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    Hunting for binary central stars of planetary nebulae: exploiting archival data
    The detection of new binary central stars of planetary nebulae is crucial to definitively determine the importance of binary interactions in the nebular...
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    Hunting for brown dwarf binaries with X-Shooter
    The refinement of the brown dwarf binary fraction may contribute to the understanding of the substellar formation mechanisms. Peculiar brown dwarf spectra or...
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    Hunting for eclipsing Post Common Envelope Binaries from SDSS
    We give an overview of a project aiming to identify new eclipsing post common envelope binaries from the Sloan Digital Sky Survey. This work focuses on the...
  • Publication
    Hunting for red supergiant binaries: UVIT photometry of the SMC
    . We present UVIT/Astrosat UV photometry of the RSG population of the Small Cloud galaxy (SMC). As RSGs are extremely faint in the far-UV, these observations...
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    Hunting for Shooting Stars in 30 Doradus
    We are undertaking an ambitious proper motion survey of massive stars in the 30 Doradus region of the Large Magellanic Cloud using the unique capabilities of...
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    HVC's Favouring Star Forming Processes in galaxy discs: a basic calculation and some recent HI observations
    Indirect evidence from detailed chemical evolution studies shows that infall of low metallicity gas appears to have proceeded at a rather constant rate during...
  • Publication
    Hybrid instrument for turbulence detection: wavefront sensing and scintillation detection in a fully automatic device
    In the planning stage of extremely large telescopes, site testing and study of high performance adaptive optics systems plays very important roles. Site testing...
  • Publication
    Hydrodynamical simulations of Multiple Shell Planetary Nebulae
    We present hydrodynamical simulations of multiple shell planetary nebulae (MSPN) formation using evolutionary models of 1, 1.5, 2, 2.5, 3.5 and 5 M_odot...