The Red Giants in NGC 6633 as Seen with CoRoT, HARPS and SOPHIE
The open cluster NGC 6633 was observed with CoRoT in 2011 and simultaneous high-resolution spectroscopy was obtained with the SOPHIE and HARPS spectrographs. One of the four targets was not found to be a cluster member. For all stars we provide estimates of the seismic and spectroscopic parameters.
KeywordsRadial Velocity Surface Gravity Cluster Member Atmospheric Parameter Radial Velocity Curve
The CoRoT space mission, launched on 2006 December 27, was developed and is operated by the CNES, with participation of the Science Programs of ESA, ESA’s RSSD, Austria, Belgium, Brazil, Germany and Spain. This work is based on observations collected at La Silla Observatory, ESO (Chile) under program LP185.D-0056.
- Baglin, A., Auvergne, M., Barge, P., et al. 2006, in ESA Special Publication, Vol. 1306, ESA Special Publication, ed. M. Fridlund, A. Baglin, J. Lochard, & L. Conroy, 33Google Scholar