Detalles de publicación
PP 022064
The homogeneity of chemical abundances in HII regions of the Magellanic Clouds
(1) INAOE, Mexico, (2) IAC, Spain, (3) ULL, Spain, (4) CIEMAT, Spain
We use very deep spectra obtained with the Ultraviolet-Visual Echelle Spectrograph at the Very Large Telescope to derive physical conditions and chemical abundances of four HII regions of the Large Magellanic Cloud (LMC) and four Hii regions of the Small Magellanic Cloud (SMC). The observations cover the spectral range 3100–10400 Å with a spectral resolution of Δ