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Table 1.

Main properties of the observed sample of SRs.

Star RA Dec Var. Period Spectral ΔmV IRAS fluxes (Jy)
Hip. dist. Gaia dist.
type (d) type (mag) 12 25 60 100 (pc) (pc)
VX And 00:19:54 +44:42:34 SRa 375 C 2.2 53 15 4 2 394 622
V465 Cas 01:18:14 +57:48:11 SRb 60 M 1.8 72 32 5 2 348 364
V370 And 01:58:44 +45:26:07 SRb 228 M 1.0 499 292 42 16 174 141
Z Eri 02:47:56 −12:27:38 SRb 80 M 1.6 63 27 4 1 256 277
RZ Ari 02:55:48 +18:19:54 SRb 57 M 0.6 147 37 6 2 108 98
SS Cep 03:49:30 +80:19:21 SRb 90 M 1.1 114 55 11 4 260 295
TT Tau 04:51:31 +28:31:37 SRb 167 C 2.0 33 11 7 4 362 727
W Ori 05:05:24 +01:10:39 SRb 212 C 4.2 184 52 14 6 377 1009
RX Lep 05:11:23 −11:50:57 SRb 60 M 2.4 280 124 19 6 149 397
Y Tau 05:45:39 +20:41:42 SRb 242 C 2.7 144 51 13 4 357 614
S Lep 06:05:45 −24:11:44 SRb 89 M 1.6 258 141 17 5 203 229
RY Mon 07:06:56 −07:33:27 SRa 456 C 1.7 59 17 5 19 433 947
RT Hya 08:29:41 −06:19:08 SRb 290 M 3.2 106 41 6 2 301 291
RT Cnc 08:58:16 +10:50:43 SRb 60 M 1.8 73 29 4 1 243 244
R Crt 11:00:34 −18:19:30 SRb 160 M 1.4 638 308 50 20 261 236
Z UMa 11:56:30 +57:52:18 SRb 196 M 3.2 64 26 4 2 356 325
BK Vir 12:30:21 +04:24:59 SRb 150 M 1.5 249 102 19 8 181 235
Y UMa 12:40:21 +55:50:48 SRb 168 M 2.1 193 91 16 7 385 309
Y CVn 12:45:08 +45:26:25 SRb 157 C 2.5 276 70 17 8 320 232
RT Vir 13:02:38 +05:11:08 SRb 155 M 1.3 462 226 39 15 135 488
SW Vir 13:14:04 −02:48:25 SRb 150 M 1.5 681 340 49 15 143 300
RX Boo 14:24:12 +25:42:13 SRb 162 M 2.7 846 419 69 26 191 128
RR UMi 14:57:35 +65:55:57 SRb 43 M 0.2 124 33 5 1 141 100
τ4 Ser 15:36:28 +15:06:05 SRb 100 M 1.2 188 91 16 6 206 293
ST Her 15:50:47 +48:28:59 SRb 148 M 1.5 199 97 17 6 293 271
X Her 16:02:39 +47:14:25 SRb 95 M 1.1 484 241 39 18 137 145
g Her 16:28:38 +41:52:54 SRb 89 M 2.0 438 149 24 7 109 122
S Dra 16:42:56 +54:54:14 SRb 136 M 1.0 131 73 12 4 411 411
FI Lyr 18:42:05 +28:57:30 SRb 146 M 0.8 93 55 7 2 358 449
S Sct 18:50:20 −07:54:27 SRb 148 C 1.3 65 17 9 14 386 373
AF Cyg 19:30:13 +46:08:52 SRb 93 M 2.0 78 34 4 1 220 257
AQ Sgr 19:34:19 −16:22:27 SRb 200 C 2.3 57 19 6 6 333 557
RT Cap 20:17:06 −21:19:04 SRb 393 C 1.2 73 21 4 4 291 429
UU Dra 20:24:04 +75:15:14 SRb 120 M 1.5 132 90 13 5 336 330
EU Del 20:37:55 +18:16:07 SRb 60 M 1.1 175 49 7 2 117 110
U Del 20:45:28 +18:05:24 SRb 110 M 1.3 142 78 11 4 481 262
IQ Aqr 20:49:17 −00:33:48 SRb 385 M 0.6 61 23 4 2 304 202
W Cyg 21:36:02 +45:22:29 SRb 131 M 2.1 349 142 22 8 175 201
RU Cyg 21:40:39 +54:19:29 SRa 233 M 2.4 190 105 18 19 249 516
EP Aqr 21:46:32 −02:12:46 SRb 55 M 0.4 637 321 47 16 114 124
TW Peg 22:03:59 +28:20:54 SRb 930 M 0.9 262 152 22 8 269 244
o1 Ori 04:52:32 +14:15:02 SRb 30 M 0.2 85 21 5 4 200 162
SV Lyn 08:03:40 +36:20:42 SRb 70 M 0.9 52 29 5 1 293 272
SV Peg 22:05:42 +35:20:55 SRb 145 M 1.8 265 146 24 10 234 890
AK Hya 08:39:53 −17:18:11 SRb 75 M 0.6 192 93 15 6 156 192
RW Boo 14:41:13 +31:34:20 SRb 209 M 1.5 61 30 5 3 293 307
IQ Her 18:17:55 +17:58:53 SRb 75 M 0.5 64 21 6 3 467 208
AA Cyg 20:04:28 +36:49:00 SRb 213 S 3.0 40 15 5 9 417 775
X Cnc 08:55:23 +17:13:53 SRb 195 C 2.0 90 25 7 3 343 898

Notes. Description of the columns from left to right. (1) GCVS designation (Samus et al. 2009; (2–3) RA and Dec (J2000); (4–7) Variability type, period of variability, spectral type, and variation amplitude from the GCVS (Samus et al. 2009); (8–11) IRAS fluxes (Helou & Walker 1988). (12) Distance derived from HIPPARCOS parallax (van Leeuwen 2007); (13) Distance derived from Gaia parallax (Gaia DR2; Gaia Collaboration 2018).

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