No CrossRef data available.
Article contents
Double-radial-mode SX Phoenicis stars in the globular clusters NGC 5466 and M71
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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 0.781, which is also consistent with the theoretical value.
- Type
- Part 3. Variable stars as tracers of different stellar populations – galactic and globular clusters, LMC/SMC and Local Group galaxies
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 166 - 170
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
Gilliland, R.L., Bono, G., Edmonds, P.D., Caputo, F., Cassisi, S., Petro, L.D., Saha, A., Shara, M.M.
1998
ApJ, 507, 818
Google Scholar
Harris, H.C.
1996
AJ, 112, 1487 (http://physun.physics.mcmaster.ca/Globular.html; revised 2003 February)Google Scholar
Pych, W., Kaluzny, J., Krzeminski, W., Schwarzenberg-Czerny, A., Thompson, I.B.
2001
A&A, 367, 148
Google Scholar
Santolamazza, P., Marconi, M., Bono, G., Caputo, F., Cassisi, S., Gilliland, R.L.
2001
ApJ, 554, 1124
Google Scholar
You have
Access