The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation [electronic resource] : Proceedings of the ESO Workshop held in Garching, Germany, 4-8 April 2005 / edited by A. Richichi, F. Delplancke, F. Paresce, A. Chelli.
Series: Eso Astrophysics Symposia, European Southern ObservatoryPublisher: Berlin, Heidelberg : Springer Berlin Heidelberg, 2008Description: XXIX, 603 p. online resourceContent type:- text
- computer
- online resource
- 9783540742562
- Popular works
- Astronomy
- Astrophysics
- Cosmology
- Physical measurements
- Measurement
- Microwaves
- Optical engineering
- Popular Science
- Popular Science in Astronomy
- Astronomy, Astrophysics and Cosmology
- Measurement Science and Instrumentation
- Microwaves, RF and Optical Engineering
- Signal, Image and Speech Processing
- 520 23
- QB1-991

The Power of Optical/IR Interferometry -- Science: Stars — stellar diameters, limb darkening, flattening, surface structures -- Science: Stars — circumstellar matter, IR objects -- Science: Science: Stars — binaries and multiples -- Science: Stars — Galactic centre, AGNs, astrometry, exo-planets and future targets -- Instrumentation: Concepts for future interferometric fringe tracking -- Instrumentation: 2nd Generation Instrumentation for the VLTI – Proposals -- Instrumentation: Concepts for future interferometric instrumentation -- Posters — Science -- Posters — Instrumentation.
Long-baseline interferometry has been traditionally regarded as a very technical method with a limited number of applications. At the turn of the millennium, with the introduction of large community-oriented facilities such as the VLTI, we are seeing a transformation into a major astronomical technique, with a corresponding dramatic increase in the number of publications. This book marks this transition, by providing a wide and deep insight into a large number of diverse and compelling results recently obtained by long-baseline interferometers. It also provides an insight into concepts which form the basis of future instruments and further developments in this technique.