Cross-correlation Method to Detect Debris Disks Below the Confusion limit in the Far IR

Details Cross-correlation Method to Detect Debris Disks Below the Confusion limit in the Far IR Cross-correlation Method to Detect Debris Disks Below the Confusion limit in the Far IR

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf...81l&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

Scientific paper

Two thirds of the stars in the vicinity of the Sun are red dwarfs and the frequency of planetary systems around them has not been estimated yet, not even preliminarily as for solar-like stars. Detection of cold dust of debris disks around these stars at submillimeter wavelengths would provide estimation of this frequency. We investigate the sensitivity of the future space missions Herschel/PACS, SAFIR and GISMO to the mass of the dust expected in these disks.

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