Title: An Enhanced Spectroscopic Census of the Orion Nebula Cluster Authors: Hillenbrand L.A., Hoffer A.S., Herczeg G.J. Table: ONC Spectral Types ================================================================================ Byte-by-byte Description of file: aj480759t2_mrt.txt -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- ID Identifier (1) 7 A1 --- f_ID [e] Flag on ID (2) 9 I1 h RAh Hour of Right Ascension (J2000) 11- 12 I2 min RAm Minute of Right Ascension (J2000) 14- 18 F5.2 s RAs Second of Right Ascension (J2000) 20 A1 --- DE- Sign of the Declination (J2000) 21 I1 deg DEd Degree of Declination (J2000) 23- 24 I2 arcmin DEm Arcminute of Declination (J2000) 26- 29 F4.1 arcsec DEs Arcsecond of Declination (J2000) 31- 96 A66 --- PSpType Previously reported spectral type (3) 98-118 A21 --- NSpType Newly reported spectral type (4) 120 A1 --- f_NSpType [f] Flag on NSpType (5) -------------------------------------------------------------------------------- Note (1): The star numbers are those listed from Jones and Walker (1988) between #1-1053, Parenago (1954) between #1054-2999, Prosser et al. (1994) for sources given as 9000+ the Prosser number, and Hillenbrand (1997) for sources given as 3000, 5000, 6000 series numbers. Note (2): e = Several optically identified objects from previous studies apparently are plate defects (JW 459, JW 699) or nebular knots (PSH 9081, PSH 9326, H97 3071, H97 3089) rather than true stellar point sources. We list them here for completeness but these sources should be removed from future list of ONC stellar objects. Note (3): The sources of the literature spectral types are as listed in Hillenbrand (1997) with more recent additions as detailed in the text. The codes are as follows: B = Blanco 1963; C = Correia et al. 2013; CK = Cohen & Kuhi 1979; D = Duncan 1993; Dae = Daemgen et al. 2012; E = Edwards et al. 1993; GS = Greenstein & Struve 1946; H = Hillenbrand 1997 and subsequent updates to electronically available table. An ``e'' indicates emission in the CaII triplet lines. A ``<'' indicates spectral type is earlier than that listed while ``>'' indicates spectral type is later than that listed; Ham = C. Hamilton 1994 unpublished masters thesis; Her = Herbig quoted in Walker 1969; HP = Herbig private communication 1996; HT = Herbig & Terndrup, 1986 or reference therein; J = Johnson 1965; LA = Levato & Abt 1976 or Abt & Levato 1977; LDW = Lallemand Duchesne, & Walker 1960; LR = Luhman, Rieke et al. 2000; Luc01 = Lucas et al. 2001 (by matching given positions to known objects of similar magnitude within 2" and translating quoted log-g=4 Teff values into a SpT using the same Teff-SpT calibration employed in Hillenbrand 1997, largely from CK); Luc06 = Lucas et al. 2006; M = McNamara 1976; P = Prosser & Stauffer private communication 1995; Par = Parenago 1954; Petal = Penston, Hunter & O'Neill 1975 or Penston, 1973; R = Rhode, Herbst & Mathieu 2001 identification of SB2's; RRL = Riddick, Roche & Lucas 2007 (by matching given positions to known objects of similar magnitude within 2"); S = Strand 1958 reference (mostly to Sharpless); Sam = A.E. Samuel 1993 unpublished PhD thesis; SBB = Smith, Beckers & Barden 1983; SHC = Slesnick, Hillenbrand & Carpenter 2004. SHC indiates optical spectral types and SHC-ir infrared spectral types; Sta = Keivan Stassun, private communication 2005, February, low dispersion spectra; Ste = Eric Stempels, private communication 2008, February, high dispersion spectra; T = Trumpler 1931; vA = van Altena et al. 1988; W = Walker 1983; WLR = Weights et al. 2009 (by matching given positions to known objects of similar magnitude within 2"; method is similar to Luc and latest types may be too late); WSH = Wolff, Strom & Hillenbrand 2004; Note (4): Spectral type derived in the present study, from the Kitt Peak/WIYN data and/or the Palomar/Norris data. Many stars were classified based on several different spectra and in the cases of disagreements multiple types are listed. Note (5): f = These sources have nebular contamination in our spectra but may include some Ca II emission contribution. -------------------------------------------------------------------------------- 3132 5 34 11.52 -5 30 19.7 M5.5 3157 5 34 11.70 -5 33 55.9 M1(H) 3126 5 34 12.91 -5 28 48.1 K7(H) 3153 5 34 13.07 -5 33 48.3 M3(H) 3156 5 34 13.22 -5 33 53.5 M2.5e(Sta) M1.5,M2e 3035 5 34 13.70 -5 17 43.8 G:(H) K4-M1 3118 5 34 14.49 -5 28 16.6 G6(H)K0(WSH) 3007 5 34 14.90 -5 14 18.0 M2.5(H) M3.5 3024 5 34 14.97 -5 15 49.3 M1(H) 3078 5 34 15.11 -5 23 00.0 M2.5 3043 5 34 15.34 -5 18 20.2 K2-K4:(H) M2(H) M5-M6 5038 5 35 00.24 -5 15 58.7 K5-K6:(H) 196 5 35 00.26 -5 18 51.0 M0(H) K7-K8,K8 194 5 35 00.41 -5 09 44.4 M5.5(H) 198 5 35 00.47 -5 25 14.2 K6e(H) 203 5 35 00.82 -5 38 08.6 M0(H) 200 5 35 00.85 -5 31 05.6 M2.5(H) M5 199 5 35 00.87 -5 09 39.2 M4(H) 201 5 35 01.03 -5 24 10.3 M2.5(H) 5084 5 35 01.07 -5 20 27.5 M3.25(RRL) M4 202 5 35 01.10 -5 23 03.8 M4.5(H) 209 5 35 01.16 -5 29 54.8 206 5 35 01.19 -5 24 06.7 M1 205 5 35 01.24 -5 21 44.4 M6(H)M7(SHC-ir) 208 5 35 01.31 -5 20 16.9 M2.5(H) 207 5 35 01.33 -5 18 21.5 M4.5 210 5 35 01.35 -5 20 22.3 K6-K8(H) M1e 204 5 35 01.45 -5 09 32.8 M1.5(H) 211 5 35 01.49 -5 28 20.6 M2.5(H) 213 5 35 01.59 -5 25 33.9 M5(H)M5.25(RRL) M5 212 5 35 01.61 -5 24 10.1 M5(H)K8(Luc01)M5(WLR) M5 216 5 35 01.62 -5 33 38.0 M3(H) 214 5 35 01.68 -5 26 36.3 M5.5(RRL) M3e 215 5 35 01.72 -5 27 09.8 M6(RRL) M4e,M4.5-M6e 218 5 35 01.83 -5 30 19.1 M4.5(H) 217 5 35 02.02 -5 18 34.3 M3(H) 219 5 35 02.09 -5 18 22.8 M5(H) M5 220 5 35 02.09 -5 26 36.1 M1.5(H)K6(Ste) 3013 5 35 02.12 -5 15 37.3 M3(H) M3.5 222 5 35 02.19 -5 29 09.5 M2(H) 3138 5 35 02.32 -5 31 10.6 M6-M8 221 5 35 02.40 -5 15 48.1 K3(H) 223b 5 35 02.40 -5 20 48.4 223a 5 35 02.44 -5 20 46.6 K5(H) 225 5 35 02.50 -5 33 09.8 M1.5(H) M2.5 227 5 35 02.70 -5 32 24.8 M5,M6 224 5 35 02.75 -5 19 44.7 M1e(H) 228 5 35 02.77 -5 32 02.6 M5e(H) M5.5 226 5 35 02.85 -5 22 08.2 G:(H) mid-K 232 5 35 03.01 -5 30 01.2 K1-K2(Sam)K4(Ste) 230 5 35 03.10 -5 22 37.8 M6(H) 229 5 35 03.17 -5 18 30.1 M1.5(H) 231 5 35 03.23 -5 17 53.5 M6(H) 5042 5 35 03.33 -5 16 22.5 234 5 35 03.44 -5 26 10.0 M4.5(H)M5.25(RRL) 233 5 35 03.45 -5 23 32.8 M3.5e(H)M6.75(RRL) 235 5 35 03.57 -5 29 26.0 M2.5e(Sta)?+M3(Dae) M1-M1.5,M2.5e 5100 5 35 03.71 -5 22 45.6 M5.5e(H)M6(SHC-ir)M5.5(RRL) M6-M7e 236 5 35 03.79 -5 24 54.0 M3e 239 5 35 03.93 -5 29 03.2 M1.5(H)M4:(E)K5,SB2(Ste) 237 5 35 03.97 -5 18 59.9 M4(H) M4 243 5 35 04.07 -5 26 37.0 M2(H) M1.5 241 5 35 04.17 -5 20 15.8 M4 244 5 35 04.17 -5 22 24.3 M5(H) M4 245 5 35 04.20 -5 26 27.7 M2e(H)M7(Luc01) 240 5 35 04.21 -5 15 21.6 M1(H) 238 5 35 04.32 -5 08 13.0 K0V(vA) 248 5 35 04.38 -5 23 13.9 M0.5-M2e(H)M1.2(P)M3(E)K4-M0(Sam)K6(Ste)M1+M7.5(C) 242 5 35 04.41 -5 08 16.9 K0 249 5 35 04.51 -5 23 56.5 K2(H)M0,M4(Sam) 250 5 35 04.51 -5 26 04.3 M3(H) 252 5 35 04.53 -5 29 38.1 K4-K5(H) 255 5 35 04.59 -5 28 26.4 K5 254 5 35 04.61 -5 26 22.8 M3(H) 251 5 35 04.62 -5 24 42.3 M2(H) 246 5 35 04.63 -5 09 53.6 M4 247 5 35 04.63 -5 09 56.0 M1.5,M4 256 5 35 04.67 -5 29 36.0 M3.5(H) 3084 5 35 04.70 -5 24 35.9 cont+emis 258 5 35 04.76 -5 26 37.8 M0.5(H) K8,M0.5 253 5 35 04.77 -5 17 42.4 K5(H)K7(Sta) K8 257 5 35 04.82 -5 22 38.8 M4.5(H) 259 5 35 04.87 -5 20 57.6 M3.5(H) 263 5 35 05.08 -5 36 44.1 M4.5(H) M5 261 5 35 05.14 -5 20 24.5 M2-M2.5e,M3e 262 5 35 05.20 -5 26 03.5 M4.5(H) M4 260 5 35 05.21 -5 14 50.5 F8(WSH)G5(S)G0+F7(Dae) 5112 5 35 05.30 -5 25 02.9 M6(Luc01)M6.5(RRL)M7.5(WLR) M4.5 271 5 35 05.34 -5 34 28.4 M0(H) 265 5 35 05.38 -5 24 10.5 M0(H) 268 5 35 05.41 -5 27 16.9 K5-K6(H)K5(Ste) 266 5 35 05.42 -5 24 15.0 M1.5,M2.5 267 5 35 05.45 -5 25 21.8 K3e 5096 5 35 05.46 -5 22 30.4 M6.5(H)M7.25(Luc01)M6.75(RRL)>M9.5(WLR) M6 270 5 35 05.47 -5 25 55.6 M3.5(H) 272 5 35 05.50 -5 27 52.0 M1.5e(H) 264 5 35 05.62 -5 11 50.9 K3-K5(H) M7 3134 5 35 09.22 -5 30 58.3 G3(Sta) K5-K8e 3166 5 35 09.26 -5 16 54.7 M2(H) 331 5 35 09.47 -5 20 58.5 M6(Luc01)M6.25(RRL)M7.5(WLR) 5127 5 35 09.51 -5 27 48.8 333 5 35 09.60 -5 27 59.8 M5-M6(H) 334 5 35 09.60 -5 28 22.8 M1e(H) 335 5 35 09.65 -5 26 23.1 M1e(H) 9001 5 35 09.68 -5 23 55.7 332 5 35 09.70 -5 21 25.0 M3.5(H) M3 336 5 35 09.77 -5 21 28.2 M0,K5-K7 337 5 35 09.77 -5 23 26.8 K8(H)K4-M0(Sam)K4(Ste) 338 5 35 09.86 -5 19 34.1 M3.5-M4(H)M3(E) 1772 5 35 09.89 -5 27 53.2 B2.5(WSH)B2Vp(Par)B2(LA)B2Vp(vA)B1-2V(J)B1.5pV(S)B3(T) 9002 5 35 09.92 -5 23 38.3 9003 5 35 09.94 -5 23 58.8 5023 5 35 09.95 -5 14 49.8 5050 5 35 10.08 -5 17 06.6 3044 5 35 10.09 -5 19 02.5 340 5 35 10.15 -5 22 32.6 M2 5129 5 35 10.16 -5 27 57.7 M1-M2 339 5 35 10.19 -5 20 21.2 M3.5(H) 3056 5 35 10.20 -5 21 00.2 M6.25(RRL) M7-M8 341 5 35 10.21 -5 23 21.4 K4-K7(H) 342 5 35 10.27 -5 21 57.0 M5(SHC-ir)M5.75(RRL) M5.5 3047 5 35 10.31 -5 19 56.1 M4.5(H) 343 5 35 10.32 -5 21 13.0 K7(H) M0 344 5 35 10.41 -5 19 52.0 M5.5 5142 5 35 10.41 -5 30 07.8 M5.5 351 5 35 10.44 -5 38 25.2 G4-G6(H) 3104 5 35 10.49 -5 26 00.2 M5.5 345 5 35 10.50 -5 22 45.5 M0.5(H)M0-M2(Sam)K6(Ste) 348 5 35 10.51 -5 26 18.1 K0(WSH)M0 392 5 35 12.70 -5 27 10.6 M6-M6.5(H) 383 5 35 12.71 -5 16 13.6 M3(H) 386 5 35 12.74 -5 16 52.9 K6-K8(H) K8 389 5 35 12.77 -5 20 35.0 M4.5-M6(H) 390 5 35 12.79 -5 20 39.1 M5(H) M3 388 5 35 12.82 -5 15 24.1 K5(H)M0.3(P)M1(E) 391 5 35 12.82 -5 20 43.6 M1e(H)M0.0(P)K0(Sam)M2(Ste)M0.5+M3.5(Dae)M0+M7(C) 398 5 35 12.85 -5 39 08.6 M0(H) K7 9024 5 35 12.88 -5 21 04.7 397 5 35 12.94 -5 28 49.8 393 5 35 13.01 -5 19 04.2 K6e(Sta) 395 5 35 13.02 -5 22 00.7 M2(H) M5.5 9025 5 35 13.03 -5 20 52.6 M8.5(RRL)>M9.5(WLR) 394 5 35 13.04 -5 20 30.3 K6(H) 402 5 35 13.05 -5 34 03.5 M5.5(H) 9029 5 35 13.06 -5 22 15.1 M4.5(H) 9028 5 35 13.09 -5 21 53.0 emis? f 9030 5 35 13.13 -5 22 52.9 M2:(H) mid-M: 9032 5 35 13.13 -5 21 13.3 M2.5e(H) M5 9031 5 35 13.15 -5 22 46.8 K:(H) 399a 5 35 13.18 -5 22 21.7 M2.5-M3 399b 5 35 13.18 -5 22 21.4 410 5 35 13.20 -5 36 18.2 M4-M5e 400 5 35 13.21 -5 20 52.8 K8-M0(H) K8-M0 401 5 35 13.21 -5 24 55.2 K0-K2e(H)G6(LR) M2e 430 5 35 13.76 -5 34 55.0 M4.5e(Sta) M4,M5 419 5 35 13.79 -5 19 25.6 M1 433 5 35 13.79 -5 39 10.8 K2-K4(P) 423 5 35 13.80 -5 22 07.0 K2e(H)M0,M4(Sam)G4-K3(LR)K5(Ste) 428 5 35 13.81 -5 30 24.2 M2.5(H) M3.5 424 5 35 13.83 -5 22 02.9 M1 427 5 35 13.83 -5 27 36.8 M4e(H) M3 425 5 35 13.90 -5 18 53.3 M1:,early-M: 9053 5 35 14.02 -5 21 23.9 429 5 35 14.05 -5 19 52.1 late-G(H)K6(Ste) 431 5 35 14.05 -5 23 38.3 M3(H)G6(LR) 489 5 35 15.80 -5 23 26.3 G4-K5(LR) 501 5 35 15.80 -5 33 12.2 M0(H) M1 1864 5 35 15.81 -5 23 09.9 B5-B8+G0-G5(Par)G4-K3(LR) 492 5 35 15.84 -5 22 45.7 M3e(H)K6-M4(LR) 1865 5 35 15.85 -5 23 14.5 O9(WSH)B2(Par)B0.5V(LA)O9V(vA)B1(J)B1(S)B1.5(T) 490 5 35 15.87 -5 20 40.5 M5(H) 494 5 35 15.87 -5 23 02.0 K7(H)K4-M2(LR) 502 5 35 15.89 -5 28 52.7 M2.5(H) 9114 5 35 15.89 -5 21 22.1 9116 5 35 15.91 -5 24 31.0 M5.5-M7(H) 9118 5 35 15.93 -5 24 17.7 cont+emis(H) cont+emis 496 5 35 15.94 -5 22 21.0 K7e(H)K-M(LR) 9119 5 35 15.94 -5 22 34.1 M2.5:e(H) M4-M6e 487 5 35 15.95 -5 14 59.1 K6(H)K5(Ste) 499 5 35 15.95 -5 23 49.7 K0:e(H)G5:(HT)G4-K5(LR)K3(Ste)M0.5+M2(Dae) 493 5 35 15.96 -5 16 57.7 M3.5 503 5 35 15.99 -5 23 52.8 F2-F7e(H)K0-K7(LR) 497 5 35 16.00 -5 21 09.9 <=K5(P) K3-K6 500 5 35 16.00 -5 21 47.0 M5.5(H) 9122 5 35 16.01 -5 20 21.0 M1.5(H) M4.5e 514 5 35 16.02 -5 39 15.1 G6(H)G8IV-V(Petal) 504a 5 35 16.06 -5 20 36.7 504b 5 35 16.06 -5 20 36.6 K2-K4(Sam) 9124 5 35 16.06 -5 25 50.8 M4(H) 1863b 5 35 16.07 -5 23 06.5 505 5 35 16.11 -5 24 10.9 M2(H) M2-M4: 1863a 5 35 16.13 -5 23 06.7 B4(Par)B3V(LA)B0V(vA)B3(J)B3(S)B6n(T) 3016 5 35 16.14 -5 15 48.2 M4 495 5 35 16.16 -5 09 19.2 M5(H) M5 506 5 35 16.18 -5 21 10.7 M5.5 9128 5 35 16.18 -5 22 55.5 M0-M3(LR) 507 5 35 16.19 -5 21 32.5 M3e(H) M4.5 509a 5 35 16.19 -5 24 55.7 509b 5 35 16.22 -5 24 55.3 9132 5 35 16.23 -5 22 37.6 M3.5(H) 3117 5 35 16.26 -5 28 33.7 M6.5 517 5 35 16.27 -5 31 00.6 M4.5(H)M4.5(Sta) 518 5 35 16.28 -5 32 02.0 M5.5(H) 512 5 35 16.29 -5 23 16.8 cont(H)K0-K7(LR) 5056 5 35 16.30 -5 17 44.1 510 5 35 16.31 -5 20 25.3 M5(H) 511b 5 35 16.31 -5 22 10.1 508 5 35 16.32 -5 15 38.2 K7-M1(H) K8 9135 5 35 16.32 -5 21 09.3 M4.5(H) 511a 5 35 16.33 -5 22 09.8 M1.5-M2e,M3-M3.5(H) 513 5 35 16.34 -5 22 48.8 M1.5e(H)K4-M2(LR) M2e,M3e 516 5 35 16.36 -5 25 09.6 M1.5(H) M0 515 5 35 16.37 -5 24 03.0 K4-K7(H)=M2(H)K-M(LR) M3e 9142 5 35 16.41 -5 21 51.0 M2.5(H) 519a 5 35 16.51 -5 22 35.1 M4(H) 1891 5 35 16.51 -5 23 22.9 O7(WSH)<09(H)O7(Par)O6:(LA)O7V(vA)O6(J)O9(T)O6(S) 519b 5 35 16.54 -5 22 35.6 9145 5 35 16.56 -5 20 40.7 521 5 35 16.58 -5 24 05.7 M0(H) M3.5e 520 5 35 16.60 -5 19 35.8 M0e(H) 527 5 35 16.61 -5 32 48.0 M0.5(H) 9147 5 35 16.62 -5 25 18.1 M2(H) 9148 5 35 16.62 -5 21 15.7 G-K:(H) 522 5 35 16.63 -5 17 23.3 9149 5 35 16.66 -5 21 31.1 3052 5 35 16.73 -5 20 19.9 M0.5 524 5 35 16.75 -5 23 16.5 G4-K5(LR) 9151 5 35 16.75 -5 22 31.4 M4(H)K-M(LR) 523 5 35 16.78 -5 16 53.5 M4.5(H) 3031 5 35 16.78 -5 17 16.7 M6-M7 526b 5 35 16.79 -5 24 04.2 526a 5 35 16.80 -5 24 04.3 K6(H)K6(E)K4III(Ham)K2-K3(Sam) 1892 5 35 16.82 -5 23 26.3 B8(Par) 529 5 35 16.88 -5 22 22.4 M0(Sam)K5-M2(LR)K5(Ste) 525 5 35 16.89 -5 17 03.2 >=M3e(H) 9153 5 35 16.91 -5 23 06.7 535 5 35 16.94 -5 25 46.9 M2.5(H) M2e,M4.5e 3055 5 35 16.95 -5 20 59.9 9155 5 35 16.96 -5 22 09.4 532 5 35 16.97 -5 22 48.5 G6(LR)K5(Ste) 531 5 35 16.98 -5 21 45.3 A0(WSH)A2V(Par)A2:V(GS)A2(T) 534 5 35 16.98 -5 23 36.9 M2e(H)K3(Ste) 528 5 35 17.00 -5 15 44.4 M5e 536 5 35 17.00 -5 22 33.0 K0-K2(H)G6(LR) 552a 5 35 17.59 -5 21 45.1 K5-K6: 552b 5 35 17.60 -5 21 45.5 553a 5 35 17.60 -5 22 56.5 K3-K4(H)>G6(LR)K5(Ste)K7(Dae) 553b 5 35 17.63 -5 22 56.6 M1(Dae) 558 5 35 17.68 -5 23 41.0 =M2(H) M5.5e 9188 5 35 17.70 -5 22 51.3 K5-M2(LR) 9189 5 35 17.70 -5 25 11.2 9191 5 35 17.73 -5 25 40.6 M4.25(RRL) 9192 5 35 17.74 -5 24 43.0 M6.5e(H) 9194 5 35 17.77 -5 23 14.5 9195 5 35 17.79 -5 23 42.2 M4-M6(LR) M3 9196 5 35 17.80 -5 23 43.9 M3-M5(LR) M5.5 562 5 35 17.81 -5 23 15.4 M0(H)K5-M2(LR) 9197 5 35 17.81 -5 22 31.3 M2-M5:(LR) 9198 5 35 17.82 -5 24 41.0 9199 5 35 17.82 -5 24 30.4 561 5 35 17.84 -5 20 54.2 G6(LR)K5(Dae) 598b 5 35 18.73 -5 22 55.7 M2(Dae) 600 5 35 18.74 -5 22 02.1 M2.5(H)K5-M2(LR)M1(SHC-ir) M1 5058 5 35 18.79 -5 18 02.8 599 5 35 18.80 -5 17 29.2 A8-F0(H) 604 5 35 18.83 -5 23 29.0 M0e(H)K4-M2(LR) G6(LR) 9245 5 35 19.09 -5 25 03.7 K7(H) 610 5 35 19.11 -5 23 26.9 K8(H)K5-M2(LR)M1(SHC-ir) K7 608 5 35 19.13 -5 20 38.8 A5(WSH)A4-A7(H)B-A(HT)B5(P) 609 5 35 19.15 -5 20 35.7 M3(H) 9246 5 35 19.15 -5 23 06.7 9248 5 35 19.17 -5 21 43.7 9249 5 35 19.19 -5 22 35.2 5147 5 35 19.21 -5 31 03.0 M6 615 5 35 19.23 -5 27 31.8 M6(H)M7(SHC-ir) 9250 5 35 19.25 -5 22 50.9 K5(H)K8-M0(H)K5-M2(LR) 612 5 35 19.29 -5 16 44.8 M3.5e(H) 613 5 35 19.29 -5 20 08.0 K2(Sam) 5040 5 35 19.33 -5 16 09.5 M2.5 5041 5 35 19.42 -5 16 08.3 616 5 35 19.49 -5 21 04.7 M3.5(H) 617 5 35 19.50 -5 22 21.4 >=M6(H) M3.5 618 5 35 19.51 -5 36 51.4 621 5 35 19.57 -5 27 35.6 M0-M3e 620 5 35 19.60 -5 23 57.2 K8(H) M0,M2 622 5 35 19.66 -5 24 26.4 M0-M2.5e(H)M0.5(P)=M5(H) 5152 5 35 20.34 -5 31 16.1 M5: 5119 5 35 20.36 -5 26 17.3 M5.5(H) 645 5 35 20.39 -5 22 13.7 mid-K(H)K5-M2(LR) M0,M1 643 5 35 20.41 -5 17 14.5 M1(H) 648b 5 35 20.45 -5 23 29.8 M3.5(Dae) 653 5 35 20.47 -5 29 11.0 M6-M6.5(H) 648a 5 35 20.49 -5 23 30.0 M0(H)M0(Dae) 650 5 35 20.52 -5 20 52.3 M3.5 9264 5 35 20.53 -5 23 31.3 652 5 35 20.54 -5 24 20.9 cont(H) 9266 5 35 20.54 -5 23 23.2 651 5 35 20.56 -5 20 43.4 M3e(Sta) 5091 5 35 20.56 -5 21 41.2 656 5 35 20.61 -5 22 55.4 M:(H)M4-M8(SHC-ir) 658 5 35 20.62 -5 24 46.3 M2e(H) 657 5 35 20.64 -5 22 45.2 M1(H) M4.5 659 5 35 20.66 -5 23 53.0 M4-M6e 660 5 35 20.71 -5 21 44.3 B3(WSH)B1(H)B8IV-V(Par)B2:Vshell(LA)B8(GS)B0Vp(J)B2(S)B8(T) 9270 5 35 20.72 -5 22 31.5 M2 3106 5 35 20.74 -5 26 15.8 655 5 35 20.75 -5 15 49.4 K0-K5:(H) 661 5 35 20.76 -5 21 55.0 M0(H)K5(Ste) 667 5 35 20.77 -5 37 54.2 M4.5(H) 662 5 35 20.81 -5 21 21.8 K7(H) K4-K6e 663 5 35 20.83 -5 21 30.1 M4.5(H) 665 5 35 20.92 -5 21 50.8 M:e(H) K-M1e 9271 5 35 20.94 -5 23 22.0 M0(H) 664 5 35 20.99 -5 16 37.7 <=K7(H)K5.5(P)K7:(E) 673 5 35 21.00 -5 31 21.5 K5(H)K5(Ste) K5 675 5 35 21.01 -5 33 39.3 K5-K7(H) M3.5 929 5 35 37.59 -5 19 44.3 M5.5(H) 933 5 35 38.03 -5 28 21.4 M4(H) 931 5 35 38.09 -5 18 11.1 mid-K 934 5 35 38.12 -5 28 33.5 M3e(H) 932 5 35 38.19 -5 14 19.0 M3-3.5(H) 936 5 35 38.34 -5 28 34.6 M3.5(H) 939 5 35 38.59 -5 27 36.9 M4.5(H) M2.5-M3.5 935 5 35 38.61 -5 09 56.6 M6.5(Sta) M6 937 5 35 38.70 -5 16 59.3 M6(H) 938 5 35 38.84 -5 12 42.0 K2(H) 943 5 35 38.93 -5 36 33.6 M5(H) 941 5 35 38.99 -5 21 01.9 K8-M0.5(H) 940 5 35 39.06 -5 08 56.2 M2II-III(?)M3:eII,III?(W) 942 5 35 39.06 -5 20 25.9 M3(H) 944 5 35 39.64 -5 27 50.3 M4(H) M3.5 3012 5 35 39.85 -5 15 49.3 M5.5 5121 5 35 39.96 -5 27 09.3 K2-K5 946 5 35 40.04 -5 26 01.2 M3.5(H) 947 5 35 40.06 -5 27 59.0 M2:(H) M3.5 945 5 35 40.16 -5 17 29.4 B6(H) 950 5 35 40.49 -5 27 02.1 948 5 35 40.60 -5 12 18.9 <=K4(H) 949 5 35 40.76 -5 09 01.4 late-K:(H)M0-M4(Her)M1(B) 952 5 35 40.84 -5 32 01.9 M2.5 951 5 35 40.89 -5 22 02.4 M4e(H) M2 955 5 35 41.28 -5 38 30.6 M4.5,M5 954 5 35 41.31 -5 27 50.4 M3(H) M3-M3.5e 953 5 35 41.35 -5 12 59.2 M2(H) 956 5 35 41.36 -5 38 34.0 M4.5 5039 5 35 41.56 -5 16 05.5 K:(H) 959 5 35 41.97 -5 28 12.7 K0(WSH)K1eIV(Par)K1eIV-V(GS)K0-1eIV(J)K3(Ste)K3+K3(Dae) 957 5 35 41.99 -5 10 11.5 K6-K8(H) 3001 5 35 42.05 -5 12 59.9 M5(Sta) M5.5 958 5 35 42.10 -5 20 05.5 M4(H) M5 960 5 35 42.27 -5 15 08.0 M0.5e(H) 962 5 35 42.47 -5 27 33.0 K6(H) 966 5 35 42.60 -5 33 49.1 M4(H) M5.5 964 5 35 42.61 -5 26 08.3 M5.5(H) 3107 5 35 42.62 -5 26 33.6 M4,M6 965 5 35 42.66 -5 25 45.1 M3.5(H) M6-M8: 961 5 35 42.75 -5 11 54.8 K6-K7(H)SB2(R) 969 5 35 42.98 -5 23 02.5 M2e(H) M1.5-M2,M2.5e 963 5 35 43.01 -5 20 13.6 K1-K2V(W)K3(S)K4IV(SBB)K5V(vA) 967 5 35 43.04 -5 13 45.5 F8IV-V(Petal)K0V(vA) 968 5 35 43.23 -5 09 17.0 K5Ve(W) 971 5 35 43.27 -5 36 28.0 K6-K8(H) 972 5 35 43.42 -5 32 44.2 M1(H) 973 5 35 43.61 -5 32 11.9 M5(H) 3030 5 35 43.67 -5 17 25.7 <=K4(H) M0.5 5109 5 35 43.77 -5 24 18.0 late-K::(H) 970 5 35 43.78 -5 09 58.8 M6.5-M7.5(H)M5.5(H) 5021 5 35 43.79 -5 14 39.3 974 5 35 44.22 -5 36 40.4 M5.5,M6.5(H)M5.5(SHC)M6-M8(SHC-ir) 976 5 35 44.35 -5 37 34.1 G6-K1,K4-K7 975 5 35 44.54 -5 32 15.7 K3:(S) 979 5 35 44.57 -5 36 33.9 M5.5(H) M5 978 5 35 44.58 -5 32 55.1 >M4(H) 980 5 35 44.83 -5 24 34.5 M4(H) M4.5 977 5 35 44.94 -5 15 20.3 K:(H) K: 982 5 35 45.38 -5 28 10.8 M1e(H) M1.5-M2e 981 5 35 45.40 -5 20 36.9 M0(H)K5,SB2?(Ste) 984 5 35 45.57 -5 28 22.9 M3(H) 983 5 35 45.62 -5 18 13.8 K2-K5 986 5 35 45.62 -5 34 08.0 3004 5 35 45.62 -5 13 36.4 M5.5 987 5 35 46.03 -5 17 49.7 M4(H) M6 985 5 35 46.10 -5 10 51.6 K7e(H) 5167 5 35 46.13 -5 34 35.8 989 5 35 46.21 -5 18 08.6 M2(H) M1.5 988 5 35 46.22 -5 15 39.9 M2e(H) 5169 5 35 46.38 -5 34 44.1 5166 5 35 46.44 -5 34 27.7 5174 5 35 46.48 -5 35 17.3 K:(H) 5175 5 35 46.58 -5 35 38.4 M5 990 5 35 46.60 -5 22 24.4 M4.5(H) M4.5-M5 991 5 35 46.82 -5 16 47.0 early-K(H) F7-K0 992 5 35 47.00 -5 17 56.8 K3-M0I(H)M0(Petal)M2:(B)K3-K5(HP)M0-M1(HP) 993 5 35 47.22 -5 17 43.6 M5(H) 995 5 35 47.37 -5 13 18.6 M1.5(H) 994 5 35 47.41 -5 10 28.4 K5-K7(H) K7,K8e 998 5 35 47.46 -5 22 49.6 M2.5(H) M2 996 5 35 47.49 -5 12 17.6 late-K:(H) K3-K5,K6 997 5 35 47.50 -5 16 58.1 F2-F7(H) 1001 5 35 47.51 -5 34 36.0 K8,K2-K6:(H) M5(H) 5016 5 35 51.93 -5 14 16.9 K:(H) 1020 5 35 52.04 -5 28 47.3 K6(H)K0(Par)K0:(J)K0:(GS) 5004 5 35 52.27 -5 13 18.6 M5(H) M5 5001 5 35 52.33 -5 12 56.9 M4(H) M4 1022 5 35 52.49 -5 27 57.5 M4.5(H) M4.5-M5 1021 5 35 52.75 -5 12 59.0 K5-K6(H) 5097 5 35 52.82 -5 22 31.4 K:(H) M1.5 1023 5 35 53.14 -5 19 30.0 M2.5(H) 1024 5 35 53.63 -5 15 41.7 K2-K3(H) 5125 5 35 53.94 -5 27 38.0 M5(H) M3 1025 5 35 54.14 -5 17 10.5 M5.5 2271 5 35 54.20 -5 37 42.8 B6(WSH)B6Veb(Par)B7eV+shell(LA)B5V(vA)B5Vne(J) 1026a 5 35 54.34 -5 26 44.6 M0.5e(H) 1026b 5 35 54.49 -5 26 45.5 1028 5 35 54.55 -5 21 57.8 K5-K6:(H) =M6(H)M5(H) 5055 5 36 27.07 -5 17 39.1 K-M1: 5111 5 36 27.18 -5 24 30.5 A0(WSH)B9V(J)B9.5V(LA) 5146 5 36 27.52 -5 30 55.6 M2.5(H) M2.5 5135 5 36 28.12 -5 28 36.5 M2.5(H) M3 5108 5 36 28.18 -5 24 17.5 G6-K0(H) 5092 5 36 28.35 -5 21 42.0 5063 5 36 28.37 -5 18 31.2 M2(H) M4.5 5093 5 36 28.44 -5 21 42.0 5018 5 36 28.72 -5 14 25.0 K5 5022 5 36 28.92 -5 14 43.2 M4.5(H) 5079 5 36 29.74 -5 20 06.8 M1(H) M0.5 5153 5 36 29.98 -5 31 20.1 K:(H) 5078 5 36 30.15 -5 20 05.9 M1(Sta) K8 5118 5 36 30.16 -5 26 12.3 M0.5(H) M0,M1 5044 5 36 30.93 -5 16 28.1 M4(H) M5.5 5117 5 36 31.51 -5 25 59.8 M5(H)M7(Sta) M7-M9