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Detailed chemical abundances for twenty one elements are presented for four red giants in the anomalous outer halo globular cluster Palomar 1 ($R_{\rm{GC}} = 17.2$ kpc, $Z=3.6$ kpc) using high-resolut...
Integral field spectroscopy of the LV2 proplyd is presented taken with the VLT/FLAMES Argus array at an angular resolution of 0.31x0.31 arcsec^2 and velocity resolutions down to 2 km/s per pixel. Foll...
Context. Palomar 1 is a peculiar globular cluster (GC). It is the youngest Galactic GC and it has been tentatively associated to several of the substructures recently discovered in the Milky Way (MW),...
In this work we have used 3D hydrodynamical (CO5BOLD) and 1D hydrostatic (LHD) stellar atmosphere models to study the importance of convection and horizontal temperature inhomogeneities in stellar abu...
We investigate the influence of convection on the formation of molecular spectral lines in the atmospheres of late-type giants. For this purpose we use the 3D hydrodynamical CO5BOLD and classical 1D L...
Chemical abundances in the galactic bulge:evidence for a fast enrichment。
Chemical abundances of the secondary stars in the black Hole binary a0620-00 and the neutron star binary cen x-4。
Chemical Abundances of NGC 5461 and NGC 5471 Derived from Echelle Spectrophotometry。
Temperature structure and chemical abundances in gaseous nebulae
Chemical abundances and kinematic properties of a planetary nebulae sample towards the galactic bulge。
Acomprehensive study of high metallicity giant extragalactic h ii regionschemical abundances

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