Table 1:
Basic parameters of the pulsation models and resulting
effective temperatures at the edges for fundamental and first-overtone pulsation.
Z |
M |
log L |
FOBEa |
FBEb |
FOREc |
FREd |
0.0001 |
0.60 |
1.95 |
- |
6850 |
- |
5750 |
|
|
2.05 |
- |
6750 |
- |
5650 |
|
|
2.15 |
- |
6750 |
- |
5550 |
|
0.65 |
1.91 |
6950 |
6850 |
6050 |
5750 |
|
|
2.01 |
6750 |
6850 |
6250 |
5750 |
|
|
2.11 |
- |
6750 |
- |
5550 |
0.001 |
0.50 |
2.11 |
- |
6650 |
- |
5450 |
|
0.50 |
2.41 |
- |
6350 |
- |
5150 |
|
0.55 |
1.81 |
6850 |
6850 |
6350 |
5650 |
|
|
1.91 |
- |
6850 |
- |
5550 |
|
|
2.01 |
- |
6750 |
- |
5450 |
|
0.65 |
1.81 |
7050 |
6750 |
6650 |
5750 |
|
|
1.91 |
6850 |
6750 |
6150 |
5650 |
|
|
2.01 |
6650 |
6850 |
6350 |
5650 |
0.004 |
0.55 |
1.81 |
- |
6950 |
- |
5750 |
|
|
1.91 |
- |
6850 |
- |
5650 |
|
|
2.01 |
- |
6750 |
- |
5450 |
Note: a First Overtone Blue Edge; b Fundamental Blue Edge; c First Overtone Red Edge; d Fundamental Red Edge. If no value is given at FOBE
and FORE, we found only fundamental models. A helium abundance
Y = 0.24 and a mixing-length parameter
= 1.5 has been adopted.
Mass and luminosity are in solar units.
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