Open Access

Table F.4

13 peculiar stars (Oe and Magnetic) in the sample with no spectroscopic analysis available but line-broadening analysis completed.

Name SpT LC Line v sin i [km s−1] vmac [km s−1] Epochs Notes
HD66811 O4 I(n)fp NV 198 12 7 Mag(a)
HD 148937 O6 …f?p OIII 39 76 22 Mag(b)
CPD -28 2561 O6.5 .f?p OIII 169 94 12 Mag(c)
HD 37022 O7 V p OIII 23 68 8 Mag(d) LPV
HD 108 O8 …fp_var OIII 46 86 4 Mag(e), SB1
HD 191612 O8 …f?p_var OIII 45 60 2 Mag(f), LPV
HD 226868 O9.7 Iabp_var OIII 95 70 5 Mag(g), SB1

HD39680 O6 V: [n]pe var He I 101 31 4 Oe, SB1
HD 155806 O7.5 V ((f))(e) OIII 49 103 3 Oe
HD 60848 O8: V: pe He I 136 123 3 Oe, LPV
HD 45314 O9: … npe SiIII 128 4 5 Oe, SB1
HD 24534 O9.5: … npe He I 226 3 Oe, SB1
HD 120678 O9.5 V e OIII 155 84 11 Oe, SB1

Notes. LPV: Line profile variability or plausible SB1; SB1: Confirmed SB1. See appendix A. Columns are: (1, 2) Name and spectral type from GOSC, (3) diagnostic line for line-broadening, (4) projected rotational velocity from the model fit, (5) macroturbulence, (6) epochs and (7) additional notes. Magnetic stars include reference to its magnetic detection. Mag: Magnetic. WR: Wolf-Rayet.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.