PMS binaries in southern molecular clouds observed with ADONIS + COMIC.

Physics

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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.

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