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Table 2

Results of our analysis.

Name Change Sp. r v helio Tc Tc lit. T eff log ϵ(Li) dlnP/dt P P J − K M K M bol
type type (km s-1) (K) (10-3   yr-1) (d, T05) (d)

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)

BH Cru SCh C −3.7 yes ... 3000 –0.7  +3.70 530 524.4 1.644 −8ṃ69 −5ṃ59
RU Vul SCh M2-4 −67.9 no ... 3700  ≲–1.5 −7.11 112 108.8 1.223 −6ṃ88 −3ṃ89
T UMi SCh M4-6   + 8.7 no ... 3300  ≲0.0 −8.47 240 229.1 1.553 −7ṃ44 −4ṃ36

R Aql CCh M5-9  +59.3 no prob1 3000  ≲0.0 −1.56  +270 270.6 1.361 −7ṃ68 −4ṃ81
dbfl2
no3
R Hya CCh M6-9 −15.9 yes yes4 3100  ≲0.0 −0.71  +385 376.6 1.261 −8ṃ16 −5ṃ17
prob2
no5
W Dra CCh M3-4  −3.6 ? ... 2950  ≲0.0  +1.03  +282 289.6 1.340 −7ṃ78 −4ṃ74

R Nor MCh M3-7 −28.5 no ... 3200  +4.6  +0.29  +510 496.2 1.310 −8ṃ55 −5ṃ50
S Her MCh M4-7.5S −17.5 yes yes2 3300  ≲0.0  +0.06 307.5 304.1 1.166 −7ṃ85 −4ṃ89
S Ori MCh M5-10  +34.5 yes dbfl2 2950  +0.8  +0.35  +430 433.4 1.352 −8ṃ39 −5ṃ49
T Cep MCh M5-9 −15.7 yes prob1 3000  +0.5  +0.12 390.9 386.6 1.328 −8ṃ19 −5ṃ16
yes2
W Hya MCh M7-9  + 40.5 no prob1 3300  +0.5 ...  +361 388.6 1.459 −8ṃ20 −5ṃ25
no6

T Her const. M2-8 −91.9 no dbfl2 3400  +2.0  +0.04 164.9 163.9 1.222 −6ṃ96 −4ṃ20

Notes. The meaning of the columns is as follows: (1) name listed in Simbad; (2) period change type; (3) range of spectral type; (4) heliocentric radial velocity; (5) presence of Tc, this paper; (6) presence of Tc, previous studies; (7) effective temperature; (8) abundance of Li; (9) rate of period change; (10) period as given in Templeton et al. (2005); (11) period found in this study; (12) mean J − K colour; (13) absolute K magnitude; (14) bolometric magnitude. References of previous studies on Tc content: Abbreviations mean: “prob” = probably, “dbfl” = doubtful.

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