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基本説明
Reprinted from ASTROPHYSICS AND SPACE SCIENCE, 286:1.
Full Description
The workshop on The Very Large Telescope Interferometer: Challenges for the Future, which was part of JENAM 2002 organised by Sociedade Portuguesa de Astronomia, took place at the Departamentos de Matematica Aplicada e Matemclt- ica Pura da Universidade do Porto (FCUP) from the 5th to the 7th of September 2002. The Very Large Telescope Interferometer (VLTI) is the major interferometric facility in the world, operated by the European Southern Observatory. It is a unique facility as it is available to the community and has a sensitivity that will bring into reach vast classes of objects in the fields of planet searches, star formation and evolution and extragalatic astrophysics. The VLTI was open to the community on a shared risk basis in March 2002. This workshop was therefore an ideal place to obtain a broad view of optical interferometry and its scientific prospects. The workshop started with a presentation of the basics of interferometry the- ory/practice, then of the VLT, Keck and LBT interferometers. The VLTI instru- ments MIDI and AMBER were introduced to its users as well as specific cal- ibration and modelling tools.
The bulk of the workshop addressed astrophysics being currently done with interferometers with very high quality reviews in the fields star formation, imaging, pulsating stars, Mira stars, active stellar shells and extragalactic astronomy. The workshop featured some talks presenting fresh VLTI data using the VINCI commissioning instrument.
Contents
Interferometry Primers.- Interferometry Theory Primer.- Optical Interferometry — A Practice Primer.- The VLTI and Other Interferometers.- The VLTI — A Status Report.- Interferometry with the Large Binocular Telescope.- VLTI Instruments and Tools.- Introducing the Near Infrared VLTI Instrument AMBER to Its Users.- Preparation of the AMBER Integrations.- MIDI — The 10 ?m Instrument on the VLTI.- Interferometric Observation at MID-Infrared Wave-Lengths with MIDI.- Genie — The Darwin Demonstrator.- PRIMA for the VLTI — Science.- The VLTI Calibrators Program: Getting Ready for High Accuracy Measurements.- 2D/3D Dust Continuum Radiative Transfer Codes to Analyze and Predict VLTI Observations.- Scientific and Technical Results from VINCI Using Coherent Estimation of Fringe Visibility.- Interferometric Science.- Probing the Close Environment of Young Stellar Objects with Interferometry.- Palomar Testbed Interferometer Observations of Young Stellar Objects.- Probing the Magnetosphere in Young Stars with AMBER/VLTI.- Unveiling the Launching Region of YSO Jets with Amber.- Imaging Stars and Their Environments with the VLTI.- Imaging with AMBER/VLTI: The Case of Microjets.- Pulsating Stars.- Cepheid Limb Darkening Models for the VLTI.- Prospects of High Angular Resolution Measurements of Binary Stars Properties with VLTI.- Interferometry: The Tool to Study Giant, Supergiant and Mira Stars.- Synthetic Radii and Visibilities for Pulsating Red Giants.- First VLTI Observations of Mira Stars.- Active Hot Star Shells.- The Wolf-Rayet Stars at High (Spatial) Resolution.- Extragalactic Astronomy with the VLTI: A New Window on the Universe.- Potential of the VLTI for Linking Stellar Frames to ICRF.- Distances on Cosmological Scales with VLTI.- The VLTI Future.- Long Range SciencePerspectives for the VLTI.- Next Generation Instrumentation for the Very Large Telescope Interferometer.- Second Generation Instrumentation for the VLTI: The French VLTI Connection.- The VLTI: Challenges for the Future.
