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Table 6.

Bolometric corrections.

Star BCHp BCBT BCVT BCJ BCH BCK BT eBT VT eVT Hp eHp J eJ H eH K eK
HD 121370 −0.115 −0.697 −0.055 1.016 1.234 1.318 3.380 0.014 2.719 0.009 2.7957 0.0004
HD 161797 −0.207 −0.984 −0.146 1.180 1.481 1.580 4.336 0.014 3.490 0.009 3.5596 0.0005
HD 175955 −0.648 −1.982 −0.618 1.482 2.056 2.209 8.513 0.016 7.146 0.010 7.1808 0.0010 4.999 0.024 4.318 0.017
HD 182736 −0.313 −1.169 −0.259 1.276 1.673 1.775 8.021 0.016 7.103 0.010 7.1673 0.0009 5.515 0.024 5.028 0.016
HD 185351 −0.372 −1.369 −0.316 1.345 1.775 1.893 6.350 0.014 5.273 0.009 5.3355 0.0005
HD 188512 −0.350 −1.257 −0.298 1.312 1.736 1.844 4.789 0.014 3.807 0.009 3.8668 0.0004
HD 189349 −0.407 −1.229 −0.358 1.251 1.675 1.778 8.411 0.016 7.411 0.010 7.4738 0.0011 5.638 0.024 5.181 0.021 5.124 0.029

Notes. Adopted bolometric corrections (BC). HIPPARCOSHp and Tycho2 BTVT magnitudes for all stars. 2MASS JHKS only if the quality is flag ‘A’ The zero-point of these bolometric corrections is set by Mbol, ⊙ = 4.75. Fbol for each star is obtained from Eq. (3) of Casagrande & VandenBerg (2018), adopting L = 3.842 × 1033 erg s−1.

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