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Table 5

Individual ages for Cepheids in NGC 1866 computed with the period-age relations of Bono et al. (2005) or Anderson et al. (2016) for fundamental pulsators, and the periods listed in Musella et al. (2016).

Cepheid Period Agea Ageb
(no rotation) (rotation: ω = 0.5ωc)
(d) (Myr) (Myr)

V6c 1.9442620 114.5 258.7
V8c 2.0070000 111.7 252.0
V5c 2.0390710 110.3 248.7
HV 12199 2.6391600 120.6 222.7
HV 12200 2.7249800 117.6 218.0
We 4 2.8603600 113.2 211.1
WS 5 2.8978000 112.1 209.3
New 2.9429300 110.8 207.1
HV 12203 2.9541100 110.4 206.6
We 8 3.0398490 108.0 202.7
We 3 3.0490400 107.7 202.3
WS 11 3.0533000 107.6 202.1
We 2 3.0548500 107.6 202.1
WS 9 3.0694500 107.2 201.4
V1 3.0845500 106.8 200.8
HV 12202 3.1012000 106.3 200.0
HV 12197 3.1437100 105.2 198.2
We 5 3.1745000 104.4 197.0
We 7 3.2322700 102.9 194.6
We 6 3.2899400 101.5 192.3
V4 3.3180000 100.9 191.3
HV 12204 3.4388200 98.1 186.8
V7 3.4520700 97.8 186.3
HV 12198 3.5228000 96.3 183.8

Notes.

(a)

Period-age relation from Bono et al. (2005).

(b)

Period-age relation from Anderson et al. (2016).

(c)

Ages computed using period-age relations for first overtone pulsators.

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