Publication type: Non-refereed

  • Publication
    The bright X ray transient GS2023+338 (=V404 Cyg) in optical outburst and decline
    The results of optical spectroscopy and photometry from La Palma (Canary Islands) of V404 Cyg are presented. They correspond to the optical counterpart of the...
  • Publication
    The Brightness Integral Equation - a Differential Approach to the Study of the Zodiacal Light
    Not Available
  • Publication
    The brown dwarf candidate [KG2001] 102 in the Cha I cloud: Is it a multiple system?
    We present deep IJHK_s and H_2 images of a region in the Chamaeleon I dark cloud containing the very low-mass young object [KG2001]102, in an attempt to search...
  • Publication
    The Buildup of E-S0 Galaxies at z < 2 from Pure Luminosity Evolution Models
    Considering that the recent history of E-S0 galaxies can be approximated by Pure Luminosity Evolution (PLE), we have examined a set of PLE models in order to...
  • Publication
    The Burst Behaviour and Evolutionary History of 4u 1820-30
    This proposal is a resubmission of an accepted RXTE AO 11 proposal. Our aim is to test evolutionary and type I burst models with the observed type I X-ray burst...
  • Publication
    The Burst Behaviour and Evolutionary History of 4u 1820-30
    This proposal is a resubmission of an accepted RXTE AO 10 proposal. Our aim is to test evolutionary and type I burst models with the observed type I X-ray burst...
  • Publication
    The Burst Behaviour and Evolutionary History of 4u 1820-30
    We want to test the observed type I X-ray burst behaviour of the bright ultra-compact binary system 4U 1820-30 with evolutionary and burst models. The short...
  • Publication
    The Ca II Infrared Triplet Lines as Diagnostics of Chromospheric Magnetism
    The Ca II infrared (IR) triplet lines are a promising candidate for studying chromospheric magnetism and dynamics. To study how good of a diagnostic the lines...
  • Publication
    The Ca Ir Triplet As A Diagnostic For Chromospheric Magnetism
    The Ca IR triplet lines are a good candidate for observing chromospheric magnetic fields. Simulations of the lines in the high-beta regime, spectropolarimetric...