Volume 464, Number 2, March III 2007
|Page(s)||687 - 695|
|Section||Stellar structure and evolution|
|Published online||11 January 2007|
Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany e-mail: firstname.lastname@example.org
2 European Southern Observatory, Karl Schwarzschild Strasse 2 , 85748 Garching bei München, Germany
Accepted: 18 December 2006
We present VLT-FORS2 optical (5700–9400 Å) spectroscopy of close (´´) companions to three nearby ( pc) Herbig Ae/Be stars (HD 144432, HD 150193, KK Oph) and one T Tauri star (S CrA). We report the detection of Li I (6707 Å) in absorption and emission lines (Hα, Ca II triplet) in the spectra of the companions. Our observations strongly suggest that the companions are physically associated pre-main-sequence stars. The spectral type derived for the companions is K5Ve for HD 144432 B, F9Ve for HD 150193 B, and G6Ve for KK Oph B. S CrA A and B were observed simultaneously. The spatially resolved spectra indicate that S CrA A (primary, north) is a G star and that S CrA B (secondary, south) is a K star. Using photometry from the literature and estimations of the R and I magnitude derived from the spectra, we localized primaries and companions in the HR diagram, derived their masses and assuming coevality constrained the age of the systems. KK Oph B (7 Myr) and S CrA B (2 Myr) are actively accreting T Tauri stars and are very likely surrounded by disks. HD 150193 B (10 Myr) and HD 144432 B (8 Myr) are weak-line T Tauri stars. Three of the four systems studied (HD 144432, HD 150193, KK Oph) have ages >7 Myr. These systems retained their disks for a longer time than typical of a young star. Our results suggest that binarity may be a key issue in understanding the lifetime of disks.
Key words: stars: binaries: visual / stars: emission-line, Be / stars: pre-main sequence / stars: fundamental parameters / planetary systems: protoplanetary disks
© ESO, 2007
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