Open Access

Table 2

Early-type star candidates.

ID RAa Deca RSgrA∗b  [1.71]  −  [2.25] c  [2.25]  −  [2.34] d Namee Typef Counterpartg
(J2000.0) (J2000.0) [′′]

1 17:45:40.047 –29:00:26.93 1.17 1.94 0.09 IRS16NW Ofpe/WN9 Bu012(E1)
2 17:45:40.122 –29:00:27.59 1.19 2.04 0.08 IRS16C Ofpe/WN9 Bu007(E1), Do129
3 17:45:40.124 –29:00:29.09 1.48 2.21 0.13 IRS16SW Ofpe/WN9 Bu015(N)
4 17:45:40.192 –29:00:27.56 2.07 1.92 0.04 IRS16CC O9.5-B0.5I Bu028(E1)
5 17:45:40.039 –29:00:30.36 2.26 2.00 0.05 IRS33N B0.5-1I Bu058(E1)
6 17:45:40.142 –29:00:30.00 2.32 1.96 0.01 E34/S2-17 B0.5-1I Bu027(E1)
7 17:45:40.094 –29:00:31.26 3.24 2.02 0.16 IRS33SE Ofpe/WN9 Bu019(E1)
8 17:45:40.165 –29:00:31.05 3.38 2.14 0.15 E47/S3-30 B0-3I Bu219(E1)
9 17:45:40.220 –29:00:30.84 3.62 3.74 0.36 IRS21 DES Bu219(E3)
10 17:45:39.864 –29:00:24.33 4.42 0.45 IRS3 DES Bu581(R)
11 17:45:39.649 –29:00:27.33 5.19 3.42 0.26 IRS6E DES Bu068(R)
12 17:45:40.455 –29:00:25.13 6.20 1.95 0.17 early(Ba) Bu123(E1)
13 17:45:39.958 –29:00:20.53 7.65 1.96 0.12 E73 O9-BI Bu085(E1)
14 17:45:40.324 –29:00:20.95 8.06 2.16 0.10 Bu169(L2)
15 17:45:40.535 –29:00:23.00 8.26 3.20 0.32 IRS10W DES,early(Ta)
16 17:45:40.343 –29:00:35.44 8.35 2.29 0.15 non-early(Ba) Bu202(L2)
17 17:45:40.039 –29:00:19.61 8.49 2.00 0.11 E75 O9-BI Bu049(E1)
18 17:45:40.098 –29:00:37.43 9.36 2.02 0.10 non-early(Ba) Bu079(E1)
19 17:45:39.324 –29:00:28.63 9.41 2.93 0.13 late(Bl) Bl103, Bu183(L1)
20 17:45:39.546 –29:00:35.01 9.47 1.93 0.16 E79 Ofpe/WN9 Bu044(E1), Do117
21 17:45:39.367 –29:00:31.57 9.49 2.06 0.11 early(Ba) Bu157(E1)
22 17:45:39.922 –29:00:18.14 10.08 1.78 0.24 IRS15SW WN8/WC9 Bu124(E1), Do124
23 17:45:40.047 –29:00:17.92 10.18 1.78 0.07 E84 O9-BI Bu051(E1)
24 17:45:39.363 –29:00:33.85 10.58 1.97 0.10 early(Ba) Bu042(E1)
25 17:45:39.506 –29:00:36.04 10.59 1.92 0.11 Bu096(E1)
26 17:45:40.144 –29:00:16.50 11.68 1.90 0.10 IRS15NE WN8/9 Bu102(E1), Do123
27 17:45:39.469 –29:00:18.61 12.09 1.77 0.03 non-early(Ba) Bu133(L1)
28 17:45:39.375 –29:00:37.21 12.61 2.16 0.07 Bu172(L1)
29 17:45:40.696 –29:00:18.36 13.00 3.74 0.32
30 17:45:40.893 –29:00:38.12 15.02 2.44 0.06 Bu185(L1)
31 17:45:39.616 –29:00:44.46 17.28 1.74 -0.02
32 17:45:40.867 –29:00:41.73 17.42 3.82 0.04 Bu480(R)
33 17:45:39.339 –29:00:09.22 21.00 2.13 0.04
34 17:45:39.475 –29:00:08.12 21.31 2.32 0.13
35 17:45:41.114 –29:00:49.62 25.72 2.68 0.02
36 17:45:42.052 –29:00:20.02 27.60 2.72 0.01
37 17:45:38.906 –29:00:03.50 28.75 2.09 0.10
38 17:45:39.603 –29:00:58.80 31.23 1.96 0.08
39 17:45:39.880 –28:59:56.49 31.68 2.03 0.05
40 17:45:39.416 –29:00:58.78 31.75 3.05 -0.03
41 17:45:41.117 –28:59:57.27 33.91 2.23 0.04
42 17:45:38.668 –28:59:57.79 35.25 1.92 0.13
43 17:45:42.266 –29:00:49.47 36.19 2.53 0.01
44 17:45:37.524 –29:00:46.02 37.56 3.84 0.01 late(Bl) Bl84
45 17:45:37.436 –29:00:08.73 39.27 2.14 0.10
46 17:45:37.122 –29:00:38.29 39.61 2.27 0.05
47 17:45:36.878 –29:00:33.15 41.79 2.15 0.03
48 17:45:40.478 –28:59:42.85 45.61 2.91 0.03
49 17:45:41.686 –29:01:08.96 46.21 2.59 0.08
50 17:45:36.561 –29:00:12.07 48.37 2.13 0.10
51 17:45:37.616 –28:59:47.42 51.63 2.49 0.00
52 17:45:35.917 –29:00:17.02 55.21 2.14 0.01
53 17:45:39.082 –28:59:33.00 56.52 1.07 0.03 fg
54 17:45:43.872 –29:00:01.32 56.96 2.27 0.05
55 17:45:40.513 –28:59:31.05 57.39 2.65 0.05
56 17:45:35.623 –29:00:11.96 60.15 2.32 0.08
57 17:45:37.013 –29:01:24.71 69.15 2.25 0.06
58 17:45:38.583 –29:01:36.43 70.95 2.20 0.08
59 17:45:41.512 –28:59:18.46 72.27 2.56 –0.01
60 17:45:41.819 –28:59:18.38 73.52 2.29 –0.00
61 17:45:44.737 –29:01:09.06 73.99 5.33 0.33
62 17:45:43.062 –28:59:24.95 74.56 2.52 0.01
63 17:45:35.700 –29:01:23.08 79.14 2.02 0.02

Notes. 

(a)

Typical positional uncertainty is (see Sect. 3.1).

(b)

Distance from Sgr A*.

(c)

Magnitude difference between [1.71]  and [2.25] , after the color correction (Sect. 3.2).

(d)

Magnitude difference between [2.25]  and [2.34] , after the color correction (Sect. 3.2) and the relative extinction correction (Sect. 3.4).

(e)

Name(s) of counterparts in Paumard et al. (2006) and Lu et al. (2009). The source # 53 is probably a foreground star, because of its very blue color in [1.71]  −  [2.25] .

(f)

Spectral type from Paumard et al. (2006), while the superscript “(Ba)” indicates the spectral type (early or non-early) from Bartko et al. (2010), “(Ta)” from Tanner et al. (2005), and “(Bl)” from Blum et al. (2003).

(g)

Counterparts from Blum et al. (2003, superscript “Bl”), Buchholz et al. (2009, superscript “Bu”) and Dong et al. (2011, superscript “Do”), and their source ID. E1, E3, L1, L2, N, and R denote quality 1 early-type candidates, quality 3 early-type candidates, quality 1 late-type candidates, quality 3 late-type candidates, sources with noisy SED, and strongly reddened sources, respectively, in Buchholz et al. (2009).

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