Physics
Scientific paper
Sep 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997msngr..89...33m&link_type=abstract
The Messenger, vol. 89, p. 33-37
Physics
1
Close Binaries: Pre-Main-Sequence Stars, Close Binaries: Molecular Clouds, Molecular Clouds: Pre-Main-Sequence Stars, Close Binaries: Energy Distribution
Scientific paper
The authors have used ADONIS + SHARP/COMIC to determine the spectral
energy distribution of close pre-main-sequence star binaries in the full
1 - 5 μm range. They have used this result to determine the physical
characteristics of both components of these close binaries.
Geoffray Herve
Monin Jean-Louis
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