Classical Cepheid
Classical Cepheids (also known as Population I Cepheids, Type I Cepheids, or Delta Cephei variables) are a type of Cepheid variable star. They are population I variable stars that exhibit regular radial pulsations with periods of a few days to a few weeks and visual amplitudes from a few tenths of a magnitude to about 2 magnitudes.
Uses material from the Wikipedia article "Classical Cepheid ", which is released under the Creative Commons BY-SA 3.0.Astronomical object | Distance | Wiki | ||
---|---|---|---|---|
Delta Cephei | Classical Cepheid | F | 884 | [x] |
HD 187921 | Classical Cepheid | F | 4078 | |
HD 30282 | Classical Cepheid | F | 1177 | |
HD 316354 | Classical Cepheid | K | 1056 | |
HIP 1213 | Classical Cepheid | F | 1212 | |
HIP 77913 | Classical Cepheid | F | 1173 | |
HIP 86269 | Classical Cepheid | F | 965 | |
l Carinae | Classical Cepheid | G | 402 | [x] |
Polaris | Classical Cepheid | F | 433 | [x] |
u Carinae | Classical Cepheid | G | 95 | [x] |
v Centauri | Classical Cepheid | F | 1226 | [x] |
W Sagittarii | Classical Cepheid | G | 2078 | [x] |
x Puppis | Classical Cepheid | K | 324 | |
Y Sagittarii | Classical Cepheid | F | 1236 | [x] |