Titlebook: Science with the VLT Interferometer; Proceedings of the E Francesco Paresce Conference proceedings 1997 Springer-Verlag Berlin Heidelberg 1

glomeruli

Solar-System Observations with the VLTIrcsec or smaller. Major objectives are expected to be the search for asteroid companions, the morphological study of asteroids, satellites of outer planets and the Pluto-Charon system, and the study of distant objects. A low-resolution spectroscopic facility will be needed to provide information on the mineralogy of asteroids and satellites.

裂縫

Giant Planet Formation and the Masses of Extrasolar Planetsiant planets. It is argued, that planets with Uranus/Neptune-masses are the standard outcome of the giant planet formation process, while Jupiter-type planets require special protoplanetary nebula conditions. Finally, a hydrodynamical calculation of the formation of a giant planet at an orbital distance of 0.05 AU is presented.

Costume

On the Detection of Exo-zodiacal Light by Nulling Interferometry with the Magellan Telescopesgh on-axis rejection ability, for the central star, and very good detection sensitivity at 10 μm wavelength, for the zodiacal thermal emission. In its non-nulling mode, working in the range 1 to 10 μm, the interferometer could address a wide range of astrophysical issues.

無意

rectocele

人充滿活力

生命

https://doi.org/10.1007/978-3-540-69398-7Population; active galactic nuclei; astrometry; astronomy; cosmology; extrasolar planet; galaxy; interferom

大范圍流行

FAWN

Flinch

Interferometry in Practicenterferometer. It touches upon sensitivity, calibration, fringe tracking, the field-of-view, synthesis imaging, and model fitting. Some examples and references to the more detailed literature are included.