Observability of extra-solar planetary disks in the mid-infrared with VLT/VISIR and NGST/MIRI

Details Observability of extra-solar planetary disks in the mid-infrared with VLT/VISIR and NGST/MIRI Observability of extra-solar planetary disks in the mid-infrared with VLT/VISIR and NGST/MIRI

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..603a&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

In the following years, new generations of mid-infrared instruments will significantly increase the number of detections of faint dust disks around close Main-Sequence stars, possibly harbouring planets. We present the results of numerical simulations that aim at determining the observability of Vega-like and Kuiper-like disks in order to infer the impact of VLT/VISIR first, and subsequently of NGST/MIRI on the study of extra-solar planetary systems.

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