Characteristics of the Galaxy according to Cepheids

Characteristics of thick disks formed through minor mergers: stellar excesses and scale lengths

Characterization of the emitting and absorbing media around the nucleus of the active galaxy UGC11763 using XMM-Newton data

Characterization of Turbulence from Submillimeter Dust Emission

Characterizing Magnetohydrodynamic Turbulence in the Small Magellanic Cloud

Characterizing Precursors to Stellar Clusters with Herschel

Characterizing the Chemistry of the Milky Way Stellar Halo: Detailed Chemical Analysis of a Metal-Poor Stellar Stream

Characterizing the Low-Mass Molecular Component in the Northern Small Magellanic Cloud

Characterizing Transition Temperature Gas in the Galactic Corona

Charge Exchange X-ray Emission of M82: Kα triplets of O VII, Ne IX, and Mg XI

Charge Exchange X-ray Emission of Nearby Star-forming Galaxies

Chemical abundance analysis of the Open Clusters Berkeley 32, NGC 752, Hyades and Praesepe

Chemical abundance analysis of the Open Clusters Cr110, NGC2099 (M37), NGC2420, NGC7789 and M67 (NGC2682)

Chemical abundance anticorrelations in globular cluster stars: The effect on cluster integrated spectra

Chemical abundance patterns in the inner Galaxy: the Scutum Red Supergiant Clusters

Chemical abundances as population tracers

Chemical abundances for 11 bulge stars from high-resolution, near-IR spectra

Chemical Abundances for Evolved Stars in M5: Lithium through Thorium

Chemical Abundances for the Outer Halo Cluster Pal 4 from Co-added High-Resolution Spectroscopy

Chemical abundances in the protoplanetary disk LV2 (Orion) - II: High dispersion VLT observations and microjet properties