| |
 |
| Paper: |
Double-radial-mode SX Phoenicis Stars in the Globular Clusters NGC 5466 and M71 |
| Volume: |
310, Variable Stars in the Local Group (IAU Colloquium 193) |
| Page: |
166 |
| Authors: |
Jeon, Y.-B.; Lee, M.G.; Kim, S.-L.; Lee, H. |
| Abstract: |
Through time-series CCD photometry of the globular cluster NGC 5466, we found three double-radial-mode SX Phe stars, all of which are consistent with the theoretical period ratio of the first overtone mode to the fundamental mode (P1H/PF); their period ratios are 0.7825, 0.7826 and 0.7919, respectively. We also detected a double-radial-mode SX Phe star in M71. Its period ratio is ).781, which is also consistent with the theoretical value. |
|
|
|
|
|
