A search for variable stars in Trumpler 24
Astronomy Group, Vrije Universiteit Brussels (VUB), Pleinlaan 2, 1050 Brussels, Belgium
2 Departamento de Física, Universidad de Concepción, Casilla 160-C Concepción, Chile
Corresponding author: J. N. Fu, email@example.com
Accepted: 2 September 2003
Trumpler 24 is a comparatively poorly-studied young open cluster. To investigate the correlation between the Be phenomenon and the cluster age, and to study the stellar variability in Trumpler 24, CCD time-series observations were made in 2001, and spectra were obtained in 2002. The results reveal 21 new variable stars, including 3 eclipsing binaries, no Be stars.
Key words: stars: variables: general / Galaxy: open clusters and associations: individual: Trumpler 24 / stars: emission-line, Be
© ESO, 2003