SCYON Abstract

Received on June 6 2007

Radial velocities of five globular clusters obtained with AAOmega

Authors	P. Székely, L.L. Kiss, K. Szatmáry, B. Csák, G.Á. Bakos, and T.R. Bedding
Affiliation	University of Szeged, Hungary University of Sydney, Australia
To appear in	Astronomische Nachrichten
Contact	pierre@physx.u-szeged.hu
URL	http://www.arxiv.org/abs/0705.3562
Links

Abstract

Using the recently commissioned multi-object spectrograph AAOmega on the 3.9m AAT we have obtained medium-resolution near-infrared spectra for 10,500 stars in and around five southern globular clusters. The targets were 47 Tuc, M12, M30, M55 and NGC 288. We have measured radial velocities to +/- 1 km/s with the cross correlation method and estimated metallicity, effective temperature, surface gravity and rotational velocity for each star by fitting synthetic model spectra. An analysis of the velocity maps and velocity dispersion of member stars revealed systemic rotation in four of the target clusters.