Titlebook: Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites; Proceedings of the E Sofia Randich,Luca Pasquini Conference pr

愉快嗎

Fluorine Abundances in the Galaxys element, that has readily observable transitions only in the infrared via vibration-rotation lines of HF. In this paper, we discuss all the available Galactic fluorine abundances to date, and add results for field stars with metallicities between [Fe/H] = -0.5 and -1.0, plus two stars that are mem

aphasia

治愈

Gleason-score

Audiometry

藐視

妨礙

braggadocio

photophobia

On the Chemical Abundances of Stars with Giant Planetshese were found to have, on average, a metal content higher than the one found in stars without detected planetary companions. In this contribution we will mainly focus on the most recent results on the chemical abundances of planet-host stars, and what kind of constraints they are bringing to the theories of planet formation.

思想流動

Chemical Composition and Kinematics of Disk Starsump stars were also observed. We determine the thin and thick properties: kinematics and chemical abundances in the solar neighbourhood. We estimate the surface mass density of the galactic disk, we also determine the thin and thick disk chemical properties.