Table 1
Sample of stars and log of the INT/IDS spectra analysed.
Star | Spectral type | M∗ | 1998 May | 1998 Jul. | 1998 Oct. | 1999 Jan. | Ntot | ||||||||||||
(M⊙) | 14 | 15 | 16 | 17 | 28 | 29 | 30 | 31 | 24 | 25 | 26 | 27 | 28 | 29 | 30 | 31 | |||
|
|||||||||||||||||||
HD 31648 | A5 Vep | 2.0 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | ... | 1 | 1 | 1 | 1 | 1 | 1 | 7 |
HD 34282 | A3 Vne | < 2.1A | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 8 |
HD 34700 | G0 IVe | 2.4B | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | ... | 1 | 1 | 1 | 7 |
HD 58647 | B9 IVep | 6.0 | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 3 |
HD 141569 | B9.5 Vev | 2.2A | 1 | 1 | 1 | 1 | ... | 1 | 1 | 1 | ... | ... | ... | ... | ... | 1 | 1 | 1 | 10 |
HD 142666 | A8 Ve | 2.0A | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | ... | ... | 1 | 1 | 1 | 11 |
HD 144432 | A9 IVev | 2.0A | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | ... | ... | 1 | 1 | 1 | 11 |
HD 150193 | A2 IVe | 2.2 | ... | 1 | 1 | 1 | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | 3 |
HD 163296 | A1 Vepv | 2.2 | 1 | 1 | 1 | 1 | 1 | 2 | 2 | 2 | ... | ... | ... | ... | ... | ... | ... | ... | 11 |
HD 179218 | A0 IVe | 2.6 | ... | 1 | 1 | 1 | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | 3 |
HD 190073 | A2 IVev | 5.1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | ... | ... | ... | ... | ... | 8 |
AS 442 | B8 Ve | 3.5 | ... | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | 5 |
VX Cas | A0 Vep | 2.3 | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | 1 | 1 | 11 |
BH Cep | F5 IIIev | 1.7A | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 2 | 2 | 2 | 2 | 1 | ... | 1 | ... | 17 |
BO Cep | F5 Ve | 1.5A | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | 1 | 13 |
SV Cep | A2 IVe | 2.4 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | 14 |
V1686 Cyg | A4 Ve | >3.5A | 1 | 1 | 1 | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | 12 |
R Mon | B8 IIIev | >5.1A | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 3 |
VY Mon | A5 Vep | >5.1A | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 3 |
51 Oph | B9.5 IIIe | 4.2 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | ... | ... | ... | ... | ... | 8 |
KK Oph | A8 Vev | 2.2A | 1 | 1 | 1 | 3 | 1 | 1 | 1 | 1 | ... | ... | ... | ... | ... | ... | ... | ... | 10 |
T Ori | A3 IVev | 2.4 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | ... | 1 | 1 | 1 | 1 | 1 | 7 |
BF Ori | A2 IVev | 2.6 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 2 | 9 |
CO Ori | F7 Vev | >3.6A | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 8 |
HK Ori | G1 Ve | 3.0A | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 8 |
NV Ori | F6 IIIev | 2.2 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 8 |
RY Ori | F6 Vev | 2.5A | ... | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 7 |
UX Ori | A4 IVe | 2.3 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 2 | 2 | 2 | 1 | 1 | 2 | 4 | 15 |
V346 Ori | A2 IV | 2.5 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 8 |
V350 Ori | A2 IVe | 2.2 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | ... | 1 | 1 | 1 | 1 | 1 | 1 | 7 |
XY Per | A2 IV | 2.8 | ... | ... | ... | ... | 1 | 1 | 1 | 1 | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 11 |
VV Ser | A0 Vevp | 4.0 | ... | 1 | 1 | 1 | 1 | 3 | 3 | 3 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | 18 |
CQ Tau | F5 IVe | 1.5B | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 8 |
RR Tau | A0 IVev | 5.8 | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 8 |
RY Tau | F8 IIIev | 1.3C | ... | ... | ... | ... | ... | ... | ... | ... | 1 | 1 | 1 | 1 | ... | 1 | 1 | ... | 6 |
PX Vul | F3 Ve | 1.5A | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | 9 |
WW Vul | A2 IVe | 2.5 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | 13 |
LkHa 234 | B5 Vev | > 5.3A | ... | ... | ... | ... | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | 1 | ... | ... | ... | 9 |
Notes. Left side: spectral types are from Mora et al. (2001). The non-flagged stellar masses are from Montesinos et al. (2009) and references therein. Flagged numbers are from Uncertainties for the stellar mass can be found in some of the references and are around 12%. Right side: the number of spectra per star is given for each observing day. The last column indicates the total number of spectra per object.
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