Brown dwarfs in young open clusters

Details Brown dwarfs in young open clusters Brown dwarfs in young open clusters

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..251m&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

3

Scientific paper

From the detection of several tens of brown dwarfs in young open
clusters (Pleiades, NGC 2516, Blanco 1), we derived new estimates of the
substellar mass function down to 30 Jupiter masses (0.03 solar masses).
Implications for the brown dwarf formation process and for the
universality of the IMF will be discussed.

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