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

Dangle

書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites影響因子(影響力)




書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites影響因子(影響力)學科排名




書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites網(wǎng)絡公開度




書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites網(wǎng)絡公開度學科排名




書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites被引頻次




書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites被引頻次學科排名




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書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites讀者反饋




書目名稱Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites讀者反饋學科排名

上流社會

Old Open Clusters as Tracers of Galactic Chemical Evolution: the BOCCE Projectmass stars and as tracers of the Galactic disk properties. Since old OCs allow us to probe the lifetime of the Milky Way disk, up to about 10 Gyr ago, they can be used to study the disk evolution withtime, and in particular its chemical history.

sundowning

Chemical Abundances and Mixing in Red Clump Stars of the Galaxyand abundances of .C, .C, N, O and other mixing sensitive chemical elements were investigated. Elemental ratios in the sample of field stars are compared to the results available for evolved stars in open clusters and to the theoretical prediction of extra mixing in stellar interiors.

TEN

Abundance Trends in the Thin and Thick Diskssurge of studies of the elemental abundance trends in the disks using high resolution spectroscopy. Here I will review and discuss the currently available data. Special focus will also be put on how we define stars to be members of either disk, and how current models of galaxy formation favour that

mortgage

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 t

comely

Observational Constraints on Nucleosynthesis in AGB Starsspite the uncertainties still existing in the chemical analysis of these stars, the determination of the abundances of several key species in their atmospheres (lithium, s-elements, carbon and magnesium isotopic ratios etc.) is an useful tool to test these theories and the mixing processes during th

comely

蒼白

A Comparison of Methods for Photospheric Abundance Determinations in K-Type Starsiques and compared the results obtained in order to establish their respective merits and faults. The two spectroscopic methods give consistent results suggesting that non- LTE effects are small, whereas the ‘mixed’ spectroscopic-photometric method leads to photospheric parameters and abundances sys

禍害隱伏

下邊深陷

NGC2324: A Relatively Young, Metal-Poor Open Cluster Located Beyond the Perseus Spiral Armtic anticentre direction. We believe that the high discrepancy in the basic cluster parameters derived in previous studies, particularly in the cluster metal content, warrants their redetermination on the basis of more reliable data.