ID | Spectral type | RA (J2000) | Dec (J2000) | Ra | Ia | Fieldb | Notesc |
W2a | B2Iae | 16 46 59.71 | -45 50 51.1 | 14.23 | 11.73 | Br. | A |
W8b | B1.5Iae | 16 47 04.95 | -45 50 26.7 | - | - | Br. | |
W13 | B0.5Ia++OBe | 16 47 06.45 | -45 50 26.0 | 14.63 | 12.06 | Br. | X, E (9.20 day) |
W21 | B0.5Iae | 16 47 01.10 | -45 51 13.6 | 15.56 | 12.74 | Br. | A |
W23a | B1.5Iae | 16 47 02.57 | -45 51 08.7 | 14.91 | 12.07 | Br. | A |
W30a | O9-B0.5Ia binf | 16 47 04.11 | -45 50 39.0 | 15.80 | 13.20 | Br. | X |
W43a | B0Iae | 16 47 03.54 | -45 50 57.3 | 15.22 | 12.26 | Br. | A |
W55 | B0Iabg | 16 46 58.40 | -45 51 31.2 | 15.25 | 12.67 | Br./1 | A |
W60 | B0Iabe | 16 47 04.13 | -45 51 52.1 | 15.96 | 13.28 | Br. | A |
W71 | B2.5Iae | 16 47 08.44 | -45 50 49.3 | 14.06 | 11.16 | Br./1 | A |
W78 | B1Iae | 16 47 01.54 | -45 49 57.8 | 14.54 | 12.04 | Br. | A |
W84 | O9.5Ibe | 16 46 59.03 | -45 50 28.2 | 15.60 | 13.63 | Br. | X? |
W234 | O9.5Ib | 16 47 01.44 | -45 52 35.0 | - | - | Br./1 | |
W239 (F) | WC9dg | 16 47 05.21 | -45 52 25.0 | 15.39 | 12.90 | Br. | X, A |
W243 | LBV (A3Ia+)h | 16 47 07.55 | -45 52 28.5 | - | - | Br. | A |
W265 | F5Ia+ g | 16 47 06.26 | -45 49 23.7 | 13.62 | 10.54 | Br. | A |
W373 | B0Iab | 16 46 57.71 | -45 53 20.0 | 14.74 | 12.32 | Br. | A |
W3002 | B0Iab | 16 46 54.24 | -45 51 54.7 | - | - | Br. | |
W3003 | B0Ib | 16 47 11.60 | -45 49 22.4 | 16.21 | 13.31 | Br. | A |
W3004 | B0Iab | 16 47 13.39 | -45 49 10.5 | 15.96 | 12.99 | Br. | A |
W3005 | O9.5Ib | 16 47 01.69 | -45 52 57.8 | 15.39 | 12.97 | Br. | A |
F1d | M2II-III | 16 46 57.84 | -45 52 18.5 | - | - | Br. | Field |
W6a | O9-B0.5Ia binf | 16 47 03.04 | -45 50 23.6 | 15.80 | 13.16 | 1 | X, P (2.20 day) |
W15 | O9Ibe | 16 47 06.63 | -45 50 29.7 | 16.38 | 13.75 | 2 | X, A |
W17 | O9Iabe | 16 47 06.25 | -45 50 49.2 | 16.19 | 13.56 | 1 | X |
W57a | B4Iae | 16 47 01.35 | -45 51 45.6 | 13.83 | 11.13 | 1 | A |
a Photometric R and I-band photometric magnitudes are taken from Clark et al. (2005) or Bonanos (2007) where available. Values from Bonanos (2007) are listed in italics; b targets are listed as Br. for members of the bright list, or 1...3 for the faint target lists. The stars W6a, W15, W17 and W57a are not included in our main target list, but are discussed in the text; c stars are noted as Eclipsing, Periodic or Aperiodic variables (Bonanos 2007) and/or X-ray sources (Clark et al. 2008); d the target F1 is a foreground star, and not a member of Wd1. References: e Negueruela et al. (2009,2008); f Clark et al. (2008); g Clark et al. (2005); h Ritchie et al. (2009).
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