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Table 13
Model luminosities L, absolute V magnitudes MV, de-reddened magnitudes Vder, and asteroseismic distances from the standard distance modulus equation (d06,01) and surface brightness relation dSB.
Star | L(σL) | MV | Vder | d06 | d01 | dSB | |||||
(L⊙) | (mag) | (mag) | (pc) | (pc) | (pc) | ||||||
|
|||||||||||
C1 | 4.2 (1.1) | 3.300 | 10.814 | 318![]() |
324![]() |
318 ± 20 | |||||
C2 | 5.3 (1.1) | 2.967 | 10.785 | 366![]() |
347![]() |
371 ± 24 | |||||
C3 | 3.6 (1.2) | 3.427 | 11.787 | 470![]() |
396![]() |
475 ± 31 | |||||
C4 | 20.0 (1.1) | 1.510 | 11.927 | 1212![]() |
1068![]() |
1231 ± 95 | |||||
C5 | 7.8 (1.1) | 2.526 | 11.857 | 735![]() |
... | 741 ± 61 |
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