Infrared interferometry with ESO's VLTI: what it can do for you
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If you have a question about this talk, please contact Jane Buckle.
Since 2004, two instruments for near and mid infrared long-baseline
interferometry have been offered to the astronomical community in service
and visitor mode by ESO at its Very Large Telescope Interferometer on Cerro
Paranal, Chile. With AMBER and MIDI , high spatial as well as spectral
resolution allow the study of young stellar objects, evolved stars, stellar
disks, binaries, novae, and even AGN dust tori. I will highlight recent
science with VLTI , and discuss its current capabilities for your scientific
projects in the context of astronomical interferometry worldwide.
This talk is part of the Cavendish Astrophysics Seminars series.
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