Open Access

Table 1

Sample overview.

Star Sp. T. N epochs IR excess
B111 O4.5 V 4
B164 O6Vz 4
B215 B1 V 3 Yes
B243 B9 III 5 Yes
B253 B3-B5 III 3
RT17, Sana17 B268 B9 III 5 Yes
B275 B7 III 3 Yes
B289 O9.7V 4 Yes
B311 O8.5 Vz 4
B331 late-B 1 Yes
B337 late-B 3 Yes

326 O6 III + B1 V 3
B86 B9 III + ? 3
B93 B2V 2
B150 B5 V 3 Yes
New OB B181 O9.7 III 1
B205 B2V 3
B213 B3 III-V 1
B234 B3 III-V 1
B272 B7 III 1
CEN55 B2 III 1

B228 G-type star 3
B23 F-type star 3
Low mass B269 F-type star 2
B290 A-type star 3
B293 F-type star 2
B336 G-type star 3

Notes. The first column shows the targets included in the Sana et al. (2017) sample and the new targets from the last observing campaign separated in two groups: the O and B stars included in the analysis of this paper and the targets identified as low-mass stars. The second and third columns list the name and spectral type, Column 4 shows the number of observations for each target, and the last column indicates whether or not the stars have IR-excess. Targets in boldface are classified as binaries following the analysis in Section 3.2. Targets 326 and B86 are double-lined spectroscopic binaries (SB2).

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