Table 9: NGC 3293: observational Parameters of Target Stars. The identifications in column two are from: F, Feast (1958); T, Turner et al. (1980); HM, Herbst & Miller (1982). WFI photometry is quoted for V > 10.75$^{\rm m}$, brighter than this there were saturation problems and values are from Turner et al. and Feinstein & Marraco (1980). Radial velocities ($v_{\rm r}$) are given in  $\mbox{km~s}^{-1}$. Instrument codes refer to FEROS (F) and Giraffe (G).
ID Alias $\alpha $(2000) $\delta $(2000) V B-V Sp. type $v_{\rm r}$ Inst. Comments
3293-001 F004 10 35 49.33 -58 13 27.6 $\phantom{1}$6.52 0.00 B0 Iab 0 $\phantom{:}$ F HD 91969, CPD-57$^{\circ}$3508; H$\alpha $ = abs+em.(stellar?)
3293-002 F003 10 35 42.02 -58 11 34.8 $\phantom{1}$6.73 0.07 B0.7 Ib -7 $\phantom{:}$ F HD 91943, CPD-57$^{\circ}$3499
3293-003 F022 10 35 46.57 -58 14 11.7 $\phantom{1}$7.61 0.11 B1 III -16 $\phantom{:}$ F CPD-57$^{\circ}$3506A
3293-004 F020 10 35 57.72 -58 13 20.6 $\phantom{1}$8.03 0.02 B1 III -21 $\phantom{:}$ F CPD-57$^{\circ}$3523
3293-005 F025 10 35 56.55 -58 14 34.7 $\phantom{1}$8.12 0.08 B1 III -8 $\phantom{:}$ F CPD-57$^{\circ}$3521
3293-006 F006 10 35 58.88 -58 14 26.1 $\phantom{1}$8.21 0.07 B1 III -10 $\phantom{:}$ F CPD-57$^{\circ}$3526B
3293-007 F008 10 36 16.08 -58 16 37.9 $\phantom{1}$8.25 0.18 B1 III -16 $\phantom{:}$ F HD 92044, CPD-57$^{\circ}$3540
3293-008 F007 10 35 54.22 -58 15 26.7 $\phantom{1}$8.59 0.05 B1 III 57 $\phantom{:}$ F HD 91983, CPD-57$^{\circ}$3516
3293-009 F048 10 36 46.90 -58 17 53.3 $\phantom{1}$8.64 0.23 A7 III -5 $\phantom{:}$ F HD 92121, CPD-57$^{\circ}$3563
3293-010 F016 10 35 40.72 -58 12 44.0 $\phantom{1}$8.77 0.00 B1 III -16 $\phantom{:}$ F CPD-57$^{\circ}$3500
3293-011 F026 10 35 58.49 -58 14 14.8 $\phantom{1}$8.85 0.04 Be (B1:) - F CPD-57$^{\circ}$3526; H$\alpha $ = broad em.
3293-012 F027 10 36 01.60 -58 15 09.4 $\phantom{1}$8.95 0.06 B1 III -28 $\phantom{:}$ F HD 92007, CPD-57$^{\circ}$3527
3293-013 F005 10 36 08.34 -58 13 04.1 $\phantom{1}$9.03 -0.04 $\phantom{-}$ B1 III -60 $\phantom{:}$ F HD 92024, CPD-57$^{\circ}$3533
3293-014 F019 10 35 58.63 -58 12 32.1 $\phantom{1}$9.09 0.19 B0.5 IIIn 50 $\phantom{:}$ F CPD-57$^{\circ}$3524A
3293-015 T133 10 35 54.92 -58 12 58.9 $\phantom{1}$9.11 -0.01 $\phantom{-}$ B1 V -16 $\phantom{:}$ F CPD-57$^{\circ}$3515
3293-016 F023 10 35 48.45 -58 14 14.5 $\phantom{1}$9.21 0.03 B2.5 V -14 $\phantom{:}$ G CPD-57$^{\circ}$3506B; strongly blended
3293-017 F024 10 35 53.65 -58 14 47.6 $\phantom{1}$9.22 0.04 B1 V -4 $\phantom{:}$ F CPD-57$^{\circ}$3517
3293-018 F018 10 35 57.81 -58 12 21.1 $\phantom{1}$9.26 -0.04 $\phantom{-}$ B1 V -7 $\phantom{:}$ F CPD-57$^{\circ}$3524B
3293-019 F014 10 35 48.22 -58 12 32.9 $\phantom{1}$9.27 -0.04 $\phantom{-}$ B1 V -17 $\phantom{:}$ F CPD-57$^{\circ}$3507
3293-020 F010 10 35 30.07 -58 12 08.0 $\phantom{1}$9.55 0.03 B1.5 III -16 $\phantom{:}$ G HDE 303067
3293-021 T065 10 35 43.31 -58 13 33.4 $\phantom{1}$9.85 0.03 B1.5 III -8 $\phantom{:}$ G CPD-57$^{\circ}$3503
3293-022 F012 10 35 32.30 -58 15 22.0 $\phantom{1}$9.97 0.12 Be (B0.5-1.5n) -20 $\phantom{:}$ G HDE 303075; H$\alpha $ = twin
3293-023 T131 10 35 55.39 -58 12 19.7 10.01 -0.05 $\phantom{-}$ B1.5 III -10 $\phantom{:}$ G CPD-57$^{\circ}$3519
3293-024 F009 10 36 04.91 -58 10 43.3 10.01 -0.01 $\phantom{-}$ B1.5 III -14 $\phantom{:}$ G HDE 303065
3293-025 F015 10 35 45.17 -58 12 23.6 10.01 0.00 B2 III -18: G CPD-57$^{\circ}$3504; strongly blended
3293-026 F013 10 35 56.60 -58 11 31.4 10.16 -0.02 $\phantom{-}$ B2 III -21 $\phantom{:}$ G CPD-57$^{\circ}$3522
3293-027 T079 10 35 39.97 -58 13 56.9 10.22 0.07 Be (B0.5-1.5n) -13 $\phantom{:}$ G H$\alpha $ = abs+twin
3293-028 T132 10 35 56.61 -58 12 40.7 10.26 0.01 B2 V -10 $\phantom{:}$ G CPD-57$^{\circ}$3520
3293-029 F028 10 36 05.95 -58 14 27.0 10.32 -0.01 $\phantom{-}$ B0.5-B1.5 Vn 8 $\phantom{:}$ G CPD-57$^{\circ}$3531
3293-030 F017 10 35 53.01 -58 12 16.8 10.51 -0.04 $\phantom{-}$ B2 V -7 $\phantom{:}$ G CPD-57$^{\circ}$3514
3293-031 F033 10 36 03.51 -58 14 40.0 10.66 0.05 B2 V -7 $\phantom{:}$ G CPD-57$^{\circ}$3528
3293-032 F029 10 35 54.67 -58 13 48.6 10.69 0.01 B0.5-B1.5 Vn 0 $\phantom{:}$ G CPD-57$^{\circ}$3518
3293-033 F041 10 34 33.88 -58 12 28.2 10.72 0.66 B8 III 8 $\phantom{:}$ G HDE 303073
3293-034 T086 10 35 49.01 -58 14 54.1 10.74 0.11 B2 IIIh -16 $\phantom{:}$ G  
3293-035 F045 10 36 40.29 -58 05 54.7 10.81 0.09 B2 V -9 $\phantom{:}$ G HDE 303062
3293-036 F036 10 36 17.02 -58 08 26.5 10.90 0.19 A5 III 29: G HDE 303066
3293-037 T089 10 36 07.64 -58 15 20.2 10.94 0.04 B2 V -12: G  
3293-038 - 10 35 06.64 -58 10 34.7 11.00 -0.04 $\phantom{-}$ B2.5 V -13: G  
3293-039 F051 10 37 04.06 -58 08 01.3 11.07 0.07 A3 III 10 $\phantom{:}$ G HDE 303063
3293-040 T063 10 35 44.05 -58 13 45.9 11.21 0.05 Be (B3n) -12 $\phantom{:}$ G H$\alpha $ = abs+twin
3293-041 T087 10 35 44.66 -58 14 30.1 11.22 0.04 B2.5 V -12 $\phantom{:}$ G  
3293-042 F044 10 35 58.93 -58 05 17.8 11.27 0.11 A3 III -5 $\phantom{:}$ G HDE 303061
3293-043 T092 10 35 28.51 -58 12 49.6 11.32 0.07 B3 V 0 $\phantom{:}$ G  
3293-044 F039 10 34 38.31 -58 07 42.3 11.35 0.10 A3 III -9: G HDE 303071
3293-045 - 10 36 13.70 -58 17 32.7 11.42 0.32 Be (B1-2n) -18 $\phantom{:}$ G H$\alpha $ = twin
3293-046 F046 10 35 15.05 -58 04 26.8 11.44 0.11 A7 III 9 $\phantom{:}$ G HDE 303060
3293-047 HM322 10 35 36.62 -58 16 04.0 11.55 0.13 B2.5 V -16 $\phantom{:}$ G  
3293-048 HM292 10 35 44.99 -58 16 35.0 11.56 0.16 B2.5 V -12 $\phantom{:}$ G  
3293-049 - 10 34 20.79 -58 13 30.5 11.64 0.07 B2.5 V -18 $\phantom{:}$ G  
3293-050 T075 10 35 41.94 -58 11 56.7 11.69 0.05 B3 Vn -12 $\phantom{:}$ G  
3293-051 - 10 34 38.85 -58 07 29.7 11.73 0.20 A5 III -1 $\phantom{:}$ G  
3293-052 HM459 10 35 29.91 -58 09 28.3 11.77 0.22 A3 III -3 $\phantom{:}$ G  
3293-053 T130 10 35 50.74 -58 11 41.2 11.83 0.03 B3 V -15 $\phantom{:}$ G  
3293-054 - 10 36 25.86 -58 14 36.2 11.85 0.06 A0 III -13 $\phantom{:}$ G  
3293-055 HM212 10 36 28.66 -58 13 35.5 11.88 0.12 A3 III 1 $\phantom{:}$ G  
3293-056 - 10 35 13.55 -58 11 12.4 11.91 0.00 B3 V -2 $\phantom{:}$ G  
3293-057 T084 10 35 45.30 -58 15 28.0 11.92 0.21 B3 V -11 $\phantom{:}$ G faint companion in WFI image
3293-058 - 10 35 38.86 -58 04 26.3 11.99 0.08 A0 IIp (Si) 12 $\phantom{:}$ G  
3293-059 HM277 10 36 06.57 -58 17 53.8 12.00 0.29 B5 III-Vn 0 $\phantom{:}$ G  
3293-060 HM231 10 35 21.10 -58 12 00.5 12.02 0.07 A2 III 8 $\phantom{:}$ G  
3293-061 T052 10 35 54.72 -58 12 37.0 12.03 0.05 B5 V -14 $\phantom{:}$ G  
3293-062 HM264 10 36 05.25 -58 16 45.5 12.03 0.15 B3 V -62 $\phantom{:}$ G  
3293-063 - 10 37 04.82 -58 10 08.1 12.05 0.09 B5 V -10 $\phantom{:}$ G  
3293-064 - 10 35 54.40 -58 12 56.3 12.06 0.06 A0 II 3 $\phantom{:}$ G adjacent to T133
3293-065 - 10 34 42.02 -58 15 41.9 12.06 0.14 B5 III-V -18 $\phantom{:}$ G  
3293-066 T090 10 35 57.12 -58 15 21.6 12.07 0.16 B5 V -49: G  
3293-067 T117 10 36 13.48 -58 11 20.7 12.11 0.32 B3 V -18: G  
3293-068 - 10 35 09.57 -58 07 47.7 12.21 0.06 B9 III 12 $\phantom{:}$ G  
3293-069 HM393 10 35 24.10 -58 13 28.4 12.22 0.07 B5 V -16 $\phantom{:}$ G  
3293-070 - 10 34 54.80 -58 07 23.3 12.22 0.14 B5 III-V 12 $\phantom{:}$ G  
3293-071 - 10 34 48.62 -58 13 13.4 12.23 0.22 A7 II-III -14 $\phantom{:}$ G  
3293-072 HM408 10 35 16.11 -58 12 59.7 12.25 0.00 B8 IIp -14 $\phantom{:}$ G composite spectrum?
3293-073 - 10 35 38.51 -58 13 06.8 12.25 0.11 B6-7 V -16 $\phantom{:}$ G  
3293-074 HM403 10 35 21.96 -58 12 53.6 12.28 0.09 B8 III -16: G  
3293-075 HM299 10 35 22.72 -58 17 08.1 12.29 0.12 B5 IIIn -11 $\phantom{:}$ G  
3293-076 - 10 35 02.75 -58 13 03.4 12.29 0.34 F0 III 7 $\phantom{:}$ G  
3293-077 - 10 34 58.30 -58 11 18.6 12.32 0.20 B6-7 V -1 $\phantom{:}$ G no $\lambda $4656, 6515 data
3293-078 - 10 36 07.04 -58 05 25.6 12.36 0.13 A3 III -9 $\phantom{:}$ G  
3293-079 HM352 10 35 23.68 -58 15 06.1 12.36 0.13 A0 III -2 $\phantom{:}$ G  
3293-080 - 10 36 06.56 -58 06 55.1 12.36 0.14 B5 V -20 $\phantom{:}$ G  
3293-081 - 10 36 45.39 -58 09 50.5 12.38 0.32 A5 II -24: G  
3293-082 - 10 35 47.53 -58 05 13.3 12.40 0.21 B5 III -8: G  
3293-083 - 10 36 33.50 -58 20 33.8 12.46 0.28 A3 III 6: G  
3293-084 T093 10 36 02.29 -58 12 58.1 12.48 0.11 B5 V -17 $\phantom{:}$ G  
3293-085 - 10 36 28.00 -58 08 18.0 12.49 0.13 B5 V -10 $\phantom{:}$ G  
3293-086 - 10 35 54.92 -58 06 49.3 12.52 0.16 B5 V -13: G  
3293-087 - 10 35 04.74 -58 14 15.4 12.60 0.04 B5 V -14 $\phantom{:}$ G  
3293-088 HM401 10 35 21.74 -58 12 37.8 12.60 0.24 F0 III-V 5 $\phantom{:}$ G  
3293-089 - 10 36 50.05 -58 04 52.3 12.64 0.15 B8 III -13 $\phantom{:}$ G  
3293-090 T104 10 35 45.81 -58 16 00.0 12.67 0.31 B6-7 V -11 $\phantom{:}$ G  
3293-091 - 10 35 59.03 -58 05 53.7 12.68 0.34 A7 II -20 $\phantom{:}$ G  
3293-092 - 10 36 15.02 -58 08 04.5 12.70 0.16 B9 III -9 $\phantom{:}$ G  
3293-093 T081 10 35 35.68 -58 13 56.4 12.71 0.14 B6-7 V -12 $\phantom{:}$ G  
3293-094 T121 10 36 17.91 -58 14 29.5 12.71 0.20 B5 V -34: G  
3293-095 T120 10 36 12.90 -58 13 24.9 12.72 0.13 B6-7 V -18 $\phantom{:}$ G  
3293-096 - 10 35 03.25 -58 14 26.8 12.74 0.23 B6-7 III 12: G  
3293-097 T124 10 36 16.92 -58 15 00.0 12.75 0.13 B6-7 III -10 $\phantom{:}$ G faint companion in WFI image
3293-098 T055 10 35 52.82 -58 13 11.7 12.75 0.14 B8 III-V -13 $\phantom{:}$ G  
3293-099 - 10 36 46.36 -58 09 29.1 12.78 0.18 B5 Vn -14 $\phantom{:}$ G  
3293-100 HM313 10 35 51.31 -58 16 17.8 12.81 0.14 B6-7 III-Vn -15: G  
3293-101 - 10 36 47.50 -58 18 01.2 12.82 0.36 F0 III 16 $\phantom{:}$ G  
3293-102 - 10 34 53.56 -58 20 58.7 12.83 0.28 A2 III 16 $\phantom{:}$ G  
3293-103 - 10 34 57.00 -58 08 06.0 12.83 0.29 A7 II 2 $\phantom{:}$ G  
3293-104 T069 10 35 40.29 -58 13 01.0 12.88 0.11 B6-7 V -8: G  
3293-105 - 10 35 57.85 -58 15 02.8 12.89 0.19 B8 III-V -11 $\phantom{:}$ G  
3293-106 F034 10 35 50.51 -58 12 12.6 12.90 0.08 B6-7 V -22 $\phantom{:}$ G  
3293-107 HM243 10 36 10.82 -58 15 48.9 12.91 0.22 B8 III-V -11 $\phantom{:}$ G  
3293-108 - 10 36 09.85 -58 05 44.3 12.92 0.13 B6-7 V -6 $\phantom{:}$ G  
3293-109 HM454 10 35 32.89 -58 10 16.2 12.92 0.15 B5 V -11 $\phantom{:}$ G  
3293-110 - 10 37 02.26 -58 12 37.1 12.93 0.28 A3 II -19 $\phantom{:}$ G  
3293-111 T091 10 35 55.41 -58 15 37.1 12.96 0.16 B6-7 III-V -13 $\phantom{:}$ G  
3293-112 - 10 34 34.76 -58 16 05.0 12.99 0.18 A5 III 13: G  
3293-113 T100 10 35 58.37 -58 14 40.9 13.04 0.14 B6-7 V -16 $\phantom{:}$ G  
3293-114 - 10 36 38.81 -58 13 57.4 13.07 0.25 B6-7 III-V -15 $\phantom{:}$ G  
3293-115 - 10 35 53.98 -58 15 04.4 13.11 0.14 B8 III-V -13 $\phantom{:}$ G  
3293-116 T071 10 35 35.84 -58 13 07.6 13.12 0.11 B6-7 V -14 $\phantom{:}$ G  
3293-117 T114 10 36 09.76 -58 10 57.8 13.15 0.14 B8 III-V -8 $\phantom{:}$ G  
3293-118 - 10 35 06.71 -58 05 07.7 13.17 0.06 B8 III-V -10 $\phantom{:}$ G  
3293-119 T109 10 35 36.70 -58 15 28.2 13.18 0.22 B9 III -12 $\phantom{:}$ G  
3293-120 - 10 34 47.74 -58 07 27.4 13.20 0.33 B5 V -12: G  
3293-121 HM316 10 35 41.32 -58 15 39.2 13.23 0.21 B8: III -9 $\phantom{:}$ G  
3293-122 T119 10 36 18.64 -58 12 53.5 13.24 0.15 B9 III -12 $\phantom{:}$ G  
3293-123 - 10 35 53.12 -58 14 26.0 13.26 0.20 B8 III -27 $\phantom{:}$ G  
3293-124 - 10 35 44.93 -58 05 11.2 13.28 0.21 B8 III -9 $\phantom{:}$ G  
3293-125 T067 10 35 47.53 -58 12 46.9 13.29 0.10 B8 III-V -14: G  
3293-126 HM285 10 35 30.63 -58 17 40.4 13.29 0.22 A7 III 0 $\phantom{:}$ G  


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Target selection
3 FLAMES-Giraffe observations and data reduction
4 Spectral classification
5 Stellar radial velocities
6 Binarity
7 Summary
Appendix A: Accurate stellar cross-identifications
References
Online Material
List of tables
List of figures