Long-Term High-Precision Monitoring of Variable Stars
Volume 35 number 1 (2007)
- Gilbert Burki
- Observatoire de Genève, CH-1290 Sauverny, Switzerland
Abstract
Long-term and high-precision photometric and/or spectroscopic monitoring is required for the study of some variable stars: supergiants, slowly pulsating B-stars, stars with activity cycles and/or amplitude modulation, and so on. These observations require stable and dedicated instrumentation.