Uncertainties on the theoretical predictions for classical Cepheid pulsational quantities

G. Valle; M. Marconi; S. Degl'Innocenti; P. G. Prada Moroni

doi:10.1051/0004-6361/200912004

Free Access

Issue		A&A Volume 507, Number 3, December I 2009


Page(s)		1541 - 1554
Section		Stellar structure and evolution
DOI		https://doi.org/10.1051/0004-6361/200912004
Published online		01 October 2009

Online Material

Table 2: Coefficients of the linear analytical relations for the fundamental red and blue edges.

Table 6: ML relations for the selected cases; $\log (L/L_{\odot}) = a + b\; \log (M/M_{\odot})$ .

Table 7: Canonical $PLT_{\rm e}$ relations for the selected cases; $\log P = a + b\; \log(L/L_{\odot}) + c\; (\log T_{\rm e})$ .

Table 10: Theoretical linear period-luminosity relations in different photometric bands for individual cases.

Table 12: Theoretical quadratic period-luminosity relations for fundamental pulsators in the various individual cases.

Table 14: Non canonical $PLT_{\rm e}$ relations: $\log P = a + b\; \log(L/L_{\odot}) + c\; (\log T_{\rm e})$ .

Table 15: Theoretical linear period-luminosity relations for the fundamental noncanonical pulsators.

Table 16: Theoretical quadratic period-luminosity relations for fundamental noncanonical pulsators.

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