Volume 554, June 2013
|Number of page(s)||25|
|Section||Interstellar and circumstellar matter|
|Published online||03 June 2013|
Individual component apparent magnitudes.
Properties of individual binary and tertiary components.
Spectroscopy of all target components observed with SINFONI. The most massive component is shown at the top, the least massive component at the bottom. The most prominent absorption features of low-mass pre-main sequence stars are indicated (see Table 3 for a list). The spectra of CHXR 73 B and T 14 B are shown binned by a factor of 4.
|Open with DEXTER|
© ESO, 2013
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