Since the discovery of the first extrasolar planet 51 Pegb [1] more than 190 extrasolar planets have been detected in orbit around other stars by means of precise stellar radial velocity (RV) measurements. But all RV surveys are concentrating almost entirely on solar-type stars covering only a narrow spectral and stellar mass range (spectral type

We describe the status of a project whose main goal is to detect variability along the extreme horizontal branch of the globular cluster NGC 6752. Based on Magellan 6.5-m data, preliminary light curves are presented for some candidate variables. By combining our time-series data, we also produce a deep CMD of unprecedented quality for the cluster

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Up to now our knowledge on frequency of planets of stars that are more massive than the sun is rather limited. In here we present the discovery of a planet orbiting the F4V-F6V star 30 Ari B, which is also a member of a hierarchical triple-star system.

We present results of our projected rotational velocities (V sin i) measurements of F, G and K giants obtained from the cross-correlation function (CCF) constructed from high signal to noise spectra. We also present the calibration of the HET/HRS cross-correlation function to determine accurate projected rotational velocities V sin i for slowly

Searches for planets around evolved G-K subgiant and giant stars are essential for developing general understanding of planet formation and evolution of the planetary systems. Precise radial velocity (RV) measurements of giants have lead to the discovery of ten planets around such star. However, the long period radial velocity variations of red