arXiv · astro-ph/0004311
The Instability Strip of M3
Abstract
We present new multicolour CCD photometry of the central part of the globular cluster M3, mapping the precise position of ~120 RR Lyrae stars (RRab, RRd, RRc) on the horizontal branch (HB). The location of the double-mode variables (RRd) is in perfect agreement with recent theoretical results. We find a significant internal spread of metallicity amongst the RRab variables.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
G. Á. Bakos, J. Jurcsik. 2000-04-21. The Instability Strip of M3. https://arxiv.org/abs/astro-ph/0004311
Cite the original work for its findings. Save a collection to share your selection of sources.