On the effect of rotation on populations of classical Cepheids - I. Predictions at solar metallicity

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Table 3

Cepheid ages for three different masses and rotation rates.

	log a [yr]
	Second crossing			Third crossing

ω	0.0	0.5	0.8	0.0	0.5	0.8

5 M_⊙	8.01	8.09	8.11	8.03	8.10	8.12
7 M_⊙	7.67	7.75	7.76	7.69	7.77	7.78
9 M_⊙	7.46	7.53	7.54^*	7.48	7.55	7.56^*

Notes. The typical difference between rotating and non-rotating models is approximately 20% across the board.

^(*)

For 9 M_⊙ models, this column actually shows ω = 0.7.

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