Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
SRON Netherlands Institute for Space Research
SRON Netherlands Institute for Space Research, Netherlands and Leiden Observatory, Leiden Univ., Netherlands
SRON, PO Box 800, NL-9700 AV Groningen, The Netherlands
SRON Groningen
Leiden Observatory, Leiden / Netherlands; SRON Netherlands Institute for Space Research, Groningen / Netherlands
Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 439 92, Onsala, Sweden
ISO Science Operations Centre, Astrophysics Division, Space Science Department of ESA, Villafranca, P.O. Box 50727, 28080 Madrid, Spain. also SRON, Groningen, The Netherlands.
SRON-Groningen, The Netherlands
SRON
Space Research Organisation Netherlands, P.O.Box 800, 9700 AV Groningen, The Netherlands; ISO Data Centre, Astrophysics Division, Space Science Department of ESA, Villafranca, P.O.Box 50727, 28080 Madrid, Spain
Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, The Netherlands
SRON Netherlands Institute for Space Research, The Netherlands
ISO Data Centre, Astrophysics Division, ESA, Villafranca, Spain
Space Research Organisation Netherlands, P.O.Box 800, NL-9700 AV, Groningen, The Netherlands
MSc University of Groningen
SRON National Institute for Space Research, Groningen, The Netherlands
Space Research Organisation of The Netherlands, Postbus 800, 9700 AV, Groningen, The Netherlands
Sterrewacht Leiden, PO Box 9513, 2300 RA Leiden, The Netherlands; SRON National Institute for Space Research, PO Box 800, 9700 AV Groningen, The Netherlands
A Spitzer c2d Legacy Survey to Identify and Characterize Disks with Inner Dust Holes
A Spitzer Survey of Protoplanetary Disk Dust in the Young Serpens Cloud: How do Dust Characteristics Evolve with Time?
Absorption line diagnostics of hidden star formation in ULIRGs
Abundant crystalline silicates in the disk of a very low mass star
An outflow origin of the [NeII] emission in the T Tau triplet
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