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Table 1

Sample sources, separated according to spectral type, with variable type (V), period (P), luminosity (L), parallax (p), and distance (D).

Source V P L p D
[d] [L] [mas] [pc]

M-type stars
RX Boo SRb 162 4000 7.31 ± 0.5a 137
TX Cam M 557 8600 ··· 380
R Cas M 431 4000 5.67 ± 2.0b 176
R Dor SRb 338 4000 18.31 ± 1.0c 55
W Hya SRa 382 6000 10.18 ± 2.4b 98
R Leo M 313 2500 14.03 ± 2.7c 71
GX Mon M 527 8200 ··· 550
WX Psc M 660 10 300 ··· 700
RT Vir SRb 155 4500 7.38 ± 0.8d 226
SW Vir SRb 150 4000 6.99 ± 0.8c 143
IK Tau M 500 7700 ··· 260
CIT 4 M 534e 4000 ··· 800
IRC+10365 M 500 7700 ··· 650
IRC-10529 M 680 10 600 ··· 620
IRC-30398 M 575 8900 ··· 550
IRC+40004 M 660 10 300 ··· 600
IRC+50137 M 635 9900 ··· 1500
IRC+60169 ··· ··· 4000: ··· 400
IRC+70066 ··· ··· 4000: ··· 400
S-type stars
R And M 409 6300 ··· 350
W Aql M 490 7600 ··· 300
TV Aur SRb 182 4000: ··· 400
AA Cam Lb ··· 6000 1.28 ± 0.7c 780
S Cas M 611 8000 ··· 570
TT Cen M 462 6500 ··· 1180
T Cet SRb 159 4000 3.70 ± 0.47c 270
R Cyg M 514 8000 ··· 600
χ Cyg M 407 6500 5.53 ± 1.10c 181
R Gem M 370 5700 ··· 650
ST Her SRb 148 4000 3.41 ± 0.59c 293
Y Lyn SRc 110 4000 3.95 ± 0.95c 253
S Lyr M 438 6700 ··· 2000
RT Sco M 449 6900 ··· 400
T Sgr M 392 6000 ··· 700
DK Vul SRa 370 4000: ··· 750
EP Vul Lb ··· 4000: ··· 510
Carbon stars
LP And M 614 9600 ··· 630
V Aql SRb 353 6500 2.76 ± 0.69c 362
RV Aqr M 454 7000 ··· 550
UU Aur SRb 235 4000 ··· 240
X Cnc SRb 170 4500 2.92 ± 0.78c 342
Y CVn SRb 158 5800 3.12 ± 0.34c 321
V Cyg M 421 6000 2.73 ± 1.58c 366
RY Dra SRb 173 4500 2.32 ± 0.59c 431
UX Dra SRb 168 4000 2.59 ± 0.29c 386
U Hya SRb 450 4000 4.80 ± 0.23c 208
CW Leo M 630 9800 ··· 120
R Lep M 432 5500 2.42 ± 1.02c 413
RW LMi M 640 10 000 ··· 400
T Lyr Lb ··· 9000 1.39 ± 0.49c 719
W Ori SRb 212 7000 2.65 ± 0.95c 377
V384 Per M 535 8300 ··· 600
AQ Sgr SRb 200 3000 3.00 ± 0.67c 333
AFGL 3068 M 696 10 900 ··· 1300
IRAS 15194-5115 M 575 8900 ··· 500

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