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Search for Sub-Stellar Companions Using AO – First Results Obtained with NAOS-CONICA
We present first results of our NAOS-CONICA search for close substellar companions around young nearby stars. This program was started only a few... -
Near-Infrared AO Spectroscopy of Edge-On Protoplanetary Disks with Subaru IRCS
We carried out near infrared (1.4–4.2 μm) AO imaging and spectroscopy of two edge-on protoplanetary disks; HK TauB and HV TauC located in Taurus... -
A Search for Close Companions in Sco OB2
Using adaptive optics we study the binary population in the nearby OB association Scorpius OB2. We present the first results of our near-infrared... -
Adaptive Optics Observations of Stars in Globular Clusters and Nearby Galaxies
Observations of nearby stellar systems with the Canada-France-Hawaii Telescope PUEO Adaptive Optics system, the University of Hawaii HOKUPA’A system... -
NACO Observations of NGC 1068
We present various recent results obtained with adaptive optics systems on the very central region of NGC 1068: Grif long-slit spectroscopy in K band... -
A Near-Infrared Adaptive Optics Imaging Survey of Nearby QSOs
We present the results of a near-IR Adaptive Optics imaging survey of 32 nearby (z<0.325) QSOs with curvature AO systems on the Gemini North and... -
Subaru Deep Field with Adaptive Optics
A deep K′-band (2.12μ m) image of 1′ × 1′ blank sky field (Subaru Deep Field; SDF) taken with Subaru Adaptive Optics System (AO) is presented. The... -
Adaptive Optics Science with the MMT Adaptive Secondary: Mid-IR AO Imaging of the Post-AGB Star AC Her
The world’s first adaptive secondary has been commissioned at the 6.5m MMT. Early science results suggests that it is unique and highly productive.... -
One Year of NACO Operations
The first ESO adaptive optics system instrument, NACO, installed at the VLT has been offered to the astronomical community and used on a regular... -
T Tauri Stars in the Large Magellanic Cloud: A Combined HST and VLT Effort
The combination of the unprecedented spatial resolution attainable with WFPC2 on board HST and of the large collecting area of the VLT makes it... -
Into the Twilight Zone: Reaching the Jet Engine with AMBER/VLTI
It is currently unknown if pre-main-sequence jets originate in the star, the star-disk interaction zone or the disk. A major constraint for... -
Imaging with the VLT
For each of the four VLT unit telescopes there are at least three instruments. Already in operation for a couple of years are FORS1, FORS2 and ISAAC.... -
From the Sun to Jupiter: Evolution of Low Mass Stars and Brown Dwarfs down to Planetary Masses
We present current models for low mass stars and substellar objects down to planetary masses and discuss the success and remaining uncertainties of... -
VLT/FORS Spectroscopy in $\sigma$ Orionis: Isolated Planetary Mass Candidate Members
We present low resolution optical spectra of isolated planetary candidate members of the young cluster... -
Submm and MIR Imaging of Protostellar Clusters
The detection of protostars is achieved most efficiently at submm wavelengths. With the advent of large bolometer arrays, groups and clusters of... -
Core Collapse and the Formation of Binaries
We examine the effect of an initial turbulent velocity field on the line-of-sight properties of cloud cores, their collapse and their fragmentation... -
Physical Properties of Prestellar Cores
We present a brief summary of current progress on research into the physical and chemical properties of pre-protostellar cores. In particular, we... -
NIR Low-Resolution Spectroscopy of L-Dwarfs: An Efficient Classification Scheme for Faint Dwarfs
We present complete near infrared (0.85-2.45 μm), low-resolution ( $\sim$... -
Variability and Rotation in Low Mass Stars and Brown Dwarfs
The evolution of angular momentum in stars is not really understood today. In particular, very little is known about rotation of substellar objects.... -
Ices in Star-Forming Regions: First Results from VLT-ISAAC
The first results from a VLT-ISAAC program on the infrared spectroscopy of deeply-embedded young stellar objects are presented. The advent of 8-m...