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Spectral Types for Hipparcos Catalogue Entriesvizier.u- ... Spectral Types SP1 1 - 620 No. Spectral type HIP Type Source 1 F5 S 2 K3V 4 3 B9 S 4 F0V 2 5 G8III 2 6 M0V: S 7 G0 S 8 M6e–M8.5e

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  • Spectral Types for Hipparcos Catalogue Entries

  • Key to Spectral Types

    (see Fields H76–77 for details)

    The spectral type, luminosity class, and peculiarity code are given here (taken from Field H76) with the following (MK classification) designations:

    • O, B, A, F, G, K, M plus sub-type (0, 1, etc.), and sometimes intermediate sub-type (for example F7.2, F7.5, F7.7) for the spectral types of ‘normal stars’;

    • R, S, N, C for carbon stars; • DB, DA, DF, DG for white dwarfs; • WR, WN, WC for Wolf-Rayet stars.

    For the luminosity class, the following designations are used: Ia0, Ia, Iab, Ib for supergiants, II for bright giants, III for giants, IV for sub-giants, V for dwarfs. The sub-dwarfs are either noted sd followed by the spectral type, or class VI. Peculiarities of the spectra are noted in lower case letters (e for emission lines, m for enhanced metallic lines, n for nebulous lines, nn for very nebulous, p for peculiarity in the chemical composition, s for sharp lines, sh for a shell, v for variations in the spectrum, w for weak lines, etc.). CN indicates stars cyanogen abundance anomaly.

    Additional qualifiers have the following meaning: : indicates some doubt about the determination of the spectral type or luminosity class; / between two spectral types or luminosity classes indicates that the two classifications were made

    during the Michigan Spectral Survey; � between two spectral types or luminosity classes indicates that the parameter is intermediate between

    those given; + indicates composite spectra (the second spectrum is not given in these cases);

    ... indicates truncated spectra (the source catalogue gives further details, including peculiarities).

    The above description does not cover all MK designations which may be found here (and in Field H76). A more complete description can be found in the introduction to the Michigan Spectral Survey.

    Spectral types given are homogeneous for the HD and HDE numbered stars from�90� to�12� in declination (i.e. in the zones covered by the Michigan Spectral Survey, Volumes 1–4). North of �12� their quality is heterogeneous. This compilation of spectral types is provided for the convenience of the catalogue users. Although the highest quality spectral classification was selected to produce estimates of B � V and V � I where appropriate, no claims about the reliability of the spectral types are implied. For more careful use, SIMBAD or other original sources should be consulted.

    The source flag indicates the source of the spectral type, as follows: 1 : Michigan Spectral Survey, Vol. 1 (N. Houk & A.P. Cowley, 1975, Univ. Michigan); 2 : Michigan Spectral Survey, Vol. 2 (N. Houk, 1978, Univ. Michigan); 3 : Michigan Spectral Survey, Vol. 3 (N. Houk, 1982, Univ. Michigan); 4 : Michigan Spectral Survey, Vol. 4 (N. Houk & A. Smith-Moore, 1988, Univ. Michigan);

    G : updated after publication of the Hipparcos Input Catalogue; K : Fourth Edition of the General Catalogue of Variable Stars (GCVS, P.N. Kholopov (ed.), 1985, 1987,

    Moscow); S : SIMBAD; X : miscellaneous;

    : entry without corresponding information.

    Spectral types and corresponding source flags were generally taken directly from the Hipparcos Input Cat- alogue (HIC) compilation. In cases where the spectral type given here differed from the HIC value (either because it was truncated in the HIC compilation, or because it was updated following investigations in view of discordant photometric data), the flag ‘G’ has been assigned.

  • Spectral Types SP1 1 - 620

    No. Spectral type HIP Type Source

    1 F5 S 2 K3V 4 3 B9 S 4 F0V 2 5 G8III 2

    6 M0V: S 7 G0 S 8 M6e–M8.5e Tc G 9 G5 S

    10 F6V 2

    11 A2 S 12 K4III 3 13 K0III 4 14 K0 S 15 K2 S

    17 F3V 2 18 K5 S 19 G5 S 20 G0 S 21 K2 S

    22 G8/K0III/IV 2 23 F2V X 24 G0V 4 25 G3IV X 26 F7V 4

    27 G5V 2 28 F3/F5V 2 29 G8III 2 30 A0 S 31 K2 S

    32 B8 S 33 F2 S 34 F7.5IV–V S 35 G8/K0III/IV 4 36 K0 S

    37 F0V 2 38 G6V 1 39 F3V 4 40 B... S 41 A0 S

    42 F2 S 43 G9III–IV X 44 K2 S 45 G6/G8V: 1 46 K1III 3

    47 K3V S 48 K0/K1III 2 49 F5 S 50 G1IV 1 51 K0 S

    52 A4V 1 54 M: S 55 G2IV/V 1 56 K0 S 57 K2V 1

    58 G0 S 59 B5 G 60 F2IV 1 61 K5 S 62 G8III 2

    63 B9p SiEu G 64 K2III 3 66 F2V 1 67 F5 S 68 K0 S

    69 A0 S 71 G5 S 72 G3/G5V 4 73 K2 S 74 K5 S

    75 K4III 2 76 M0 S 77 A0V 3 78 K0 S 79 F5 S

    80 G2V 4 81 G5 S 82 G5 S 83 M0 S 84 K0 S

    85 A2 S 86 B9 S 87 F5 S 88 G8III X 89 K2 S

    90 F5IV/V 2 91 K0 S 92 G8III 4 93 F8V X 94 G2 S

    95 F5V 4 96 M0 S 97 F5V 4 98 F6/F7V 1 99 C5p G

    100 G0 S 101 F5IV/V 2 102 M1III 2 103 F6V 1 104 F7V 3

    No. Spectral type HIP Type Source

    105 F0 S 106 G7II–III S 107 M2III 2 108 K3II/III 1 109 F0 S

    110 G5 S 111 M2 S 112 M1.5V: S 113 A0 S 114 G0IV X

    115 A2IV 1 116 F3V 3 117 G8III 1 118 G0 S 119 K0 S

    120 K1IIICNIV G 121 K2III X 122 K2III X 123 K0 S 124 F0III X

    125 F2V 3 126 G5 S 128 Am... X 129 F8 S 130 K0III 3

    131 A4V X 132 F0 S 133 F5IV 2 134 A0 S 135 G5 S

    136 K2III–IV X 137 B9IIIp Mn G 138 K0/K1IV 4 139 B0 S 140 F7V 1

    141 K5 S 142 K0 S 143 K3 S 144 K5 S 145 B7III–IV X

    146 A9V 3 147 K5 S 148 F8 S 149 K3 S 150 K1III 3

    151 F3IV... X 152 F5 S 153 F8 S 154 M3III X 155 A2 S

    156 B8V X 157 G5 S 158 K0III 3 159 A3 S 160 B9V 1

    161 K5 S 162 G0 S 163 A3V 3 164 G9III X 165 Ap... 4

    166 G3V 1 167 B9 S 168 R... X 169 M0V X 170 F5V 4

    171 G3V X 172 O7 X 173 A2 S 174 G9II–III X 175 G5 S

    176 K0 S 177 A1m... 4 178 F7V 3 179 G0V 4 180 K0 S

    181 M0 S 182 K0 S 183 B4V 3 184 K0 S 185 F8 S

    186 A6V X 187 G0 S 188 F5 S 189 A3 S 190 G0 S

    191 M3 S 192 G5 S 193 G8/K0III 3 194 F0V X 195 F8 S

    196 K5 S 197 K0 S 198 A0 S 199 A0 S 200 F2 S

    201 F5 S 202 F0 S 203 K0III 4 204 K3III 2 205 F2 S

    No. Spectral type HIP Type Source

    206 G0 S 207 G8III S 208 G6/G8III 1 209 A2V X 210 G0 S

    211 G8 S 213 G5 S 214 A3 S 215 M2 S 216 A0 S

    217 A0 S 218 G8III 1 219 F8 S 220 A0 S 221 F2 S

    222 K1III 2 223 G0 S 224 K0 S 225 F3/F5V 4 226 F0/F2V 4

    228 F8 S 229 A0 S 230 F2 S 231 F6/F7IV 1 232 A0V 3

    233 K0 S 234 B8 S 235 K0 S 236 K0 S 237 G8IV 2

    238 F6/F7V 4 239 F5 S 240 F8 S 241 K0 S 242 G8IV 3

    243 K0III 1 244 F8 S 245 G5 S 246 K3 S 247 F0 S

    248 F0 S 249 F8 S 250 K0 S 251 K2III 4 252 K0... S

    253 K1III 4 254 A2 S 255 F2/F3V 4 256 F0 S 257 A0V 3

    258 K0 S 259 M0 S 260 F2V 1 261 F3V 4 262 F0V X

    263 M1 S 264 K0 S 265 K5III: 1 266 K1IIICN... 4 267 F2 S

    268 K5 S 269 G5 S 270 A2 S 271 A2III 3 272 G8/K0III 3

    273 A0V X 274 B3Ia X 275 F3V 3 276 G0 S 277 F2V 3

    278 B2IVne+... X 279 B8V X 280 A2 S 281 M0 S 282 K0 S

    283 A5 S 284 G8III 1 285 K1IV/VCN... 3 286 K0 S 287 K5 S

    288 K0 S 289 K0III 2 290 F8/G0V 3 291 Ap... 3 292 A0 S

    293 F6V 1 294 F0 S 295 F0V 2 296 G8V 3 297 A2 S

    298 K0 S 299 F5V 1 300 A3 S 301 B9IVn 4 302 M4 S

    303 Am... X 304 A2 S 305 G5IV 3 306 G2V 1 307 M0 S

    No. Spectral type HIP Type Source

    308 F0 S 309 A7V X 310 G5V 2 311 F0 S 312 B0Ibp X

    313 F3/F5V 2 314 G0 S 315 F8V 1 316 F0 S 317 F0III/IV 1

    318 G8/K0IV 3 319 O8e X 320 F1: K 321 G2/G3V 3 322 G8IV X

    323 K0 S 324 F5 S 325 F8 S 326 M0 S 327 A2 S

    328 B8V 3 329 G5 S 330 A1III X 331 Gp S 332 F6V 3

    333 A1/A2IV/V 4 334 B0 S 335 A0 S 336 K5 S 337 G5 S

    338 B S 339 A1V 1 340 F6V 2 341 G8IV 4 342 G0V 4

    343 K0III 4 344 M5e–M7e G 345 A1V 3 346 K1III 1 347 B3V X

    348 G5 S 349 B8/B9V 3 351 K0V 2 354 K0 S 355 K3Ibvar X

    356 G0 S 357 F2V X 358 G8III 1 359 G3/G5III/IV 1 360 K2 S

    361 K0III 1 362 K2III 4 363 C5II G 364 K0III 4 365 B9III X

    366 K1IV 3 367 A2/A3IV 1 368 K2 S 369 K0 S 370 K1III 2

    371 M5 S 372 K0/K1III 1 373 K2 S 374 K0 S 376 K0 S

    377 B8III X 378 F5IV X 379 K1III S 380 G5 S 381 A2 S

    382 F0V 3 383 F0 S 384 A5 S 385 G5 S 386 B2 S

    387 F2 S 388 A3 S 389 A0IV 3 390 F7 K 391 G0 S

    392 F5 S 393 K0 S 394 G2V X 395 A0IV/V 3 396 K2III 3

    397 A0 S 398 B3V X 399 K4IIIb S 400 G9V X 401 K5 S

    402 F5 S 403 G3V 4 404 F8V X 405 K2 S 406 M0 S

    407 G5V 1 408 G9III X 409 F5V 1 410 G8II X 411 K5 S

    No. Spectral type HIP Type Source

    412 F5 S 413 G0V 3 414 G6III 1 415 F2 S 416 G5 S

    417 G9III: S 418 B8MNp... X 419 G8/K0V 2 420 G0V 2 422 K0 S

    423 F0 S 424 A1Vn X 425 G0V 1 426 F0 S 427 K1III 2

    428 M2 S 429 G5 S 430 K1III 3 431 F5 S 432 A2 S

    433 K2 S 434 F2V 3 435 F3/F5V 2 436 K5V X 437 G5 S

    438 G5 S 439 M2V 3 440 B9 S 441 G8III/IV 3 442 B9V 4

    443 K1III X 444 K2III 1 445 A1Vs 1 446 K0III 1 447 G4V:p X

    448 G5 S 449 G8IV 3 450 K7 S 451 G0 S 452 F8 S

    453 K0 S 454 K0III 4 456 K0III 3 457 M3III X 458 K5 S

    459 G5V 1 460 G5 S 461 F8 S 462 F5 S 463 G8III/IV 3

    464 A0 S 465 K2 S 466 K0 S 467 G5V 2 468 K0III 1

    469 K3/K4III 2 470 B1.5IV X 471 K5 S 472 K0III X 473 K2 S

    474 A0 S 475 G0 S 476 G5III S 477 A9/F0V 3 478 F3/F5V 4

    479 G5 S 480 K1III 4 481 G5 S 482 F2+... S 483 A0 S

    484 G5V 4 485 A0 S 486 F6V 1 487 G0 S 488 G5/G6V 1

    490 G0V X 491 K0 S 492 G0 S 493 F8 S 494 F8V 1

    495 K0... S 496 K5 S 497 A3 S 498 A3 S 499 G8IV/V 1

    500 M1/M2 2 501 K3III 3 502 K5III X 503 G5 S 504 K1III–IV X

    505 O6pe X 506 A2 S 507 K3III 1 508 G5 S 509 G3V 3

    510 F5 S 511 G5 S 512 B9V 3 513 K0 S 514 F2V 4

    No. Spectral type HIP Type Source

    515 F8 S 516 M1III 3 517 F5IV/V 1 518 G5V S 519 F3IV 1

    520 M... S 521

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