luminosity classes of SR/L variables Regarding the CK Ori topic, I have checked whether how many K giants or subgiants are listed in the GCVS. Hipparcos variables are disregarded. spec. ----- K0III: HERV463 SRD 8.46 (0.05) V 54.0 K0IIIea LYNST LB: 11.7 12.7 P - K0IV-V: TAUTW LB: 10.6 11.6 P - K1.5IIIb DRAVW SRD: 6.0 7.0 V 170 K2III CENV764 SRD 8.84 9.13 V - K2III OPHkappa LB: 4.1 5.0 P - K2III SGETZ SRD: 12.7 <16.0 P 270.30 K2IIIe: ORICK SR: 5.9 7.1 V 120 K2V:-K5 ARASS LB 10.2 11.5 P - K3III CENYZ SR: 10.5 11.0 P - K3III CYGT LB: 4.91 4.96 V - K4III MUSmu LB 4.6 4.8 V - K5III AQLHK LB: 8.9 10.9 P - K5III CVNAW SR: 4.72 4.81 V - K5III TAUalpha LB: 0.75 0.95 V - K8III-M LEOSY SRB 12.2 13.1 P 82 Well, low-luminosity SR/L stars are indeed rare in the GCVS, and most of them seem to be 'boring' objects (at least to human eyes) as CK Ori. Some of Hipparcos results on them (variablity taken from the Hipparcos variablity flag): V463 Her : constant 171133.6 +162439 (2000.0) 843H 0.99 HIP084096 plx=4.24(1.13) (0.01 0.01) VW Dra: constant 171629.4 +604014 (2000.0) 632H 1.09 HIP084496 plx=6.76(0.54) (0.00 0.01) V764 Cen: small-amplitude variable 133608.3 -332844 (2000.0) 905HV2 1.21 HIP066358 plx=1.97(1.19) (0.02 0.03) U 9.11-9.29 kappa Oph: constant 165740.2 +092230 (2000.0) 319H 1.16 HIP083000 plx=37.99(0.75) (0.00 0.43) CK Ori: constant 053019.9 +041217 (2000.0) 621H 1.28 HIP025785 plx=5.68(0.85) (0.00 0.01) SS Ara: constant 175819.1 -500939 (2000.0) 930H 0.89 HIP087980 plx=2.12(1.56) (0.02 0.51) T Cyg: constant 204710.7 +342226 (2000.0) 493H 1.29 HIP102571 plx=8.18(0.55) (0.00 0.00) mu Mus: small-amplitude variable 114814.4 -664853 (2000.0) 475HV1 1.52 HIP057581 plx=7.55(0.52) (0.00 0.06) M 4.85-4.87 It would be also interesting to note some A stars are listed as SR or L in the GCVS. A/Fe-K CRAQT SRD: 11.4 12.5 P 79.145 A0IV NORNS SR: 11.5 12.0 P 130 A6 GEMYZ L: 10.8 11.6 P - Regards, Taichi Kato