Titlebook: New Quests in Stellar Astrophysics II; Ultraviolet Properti Miguel‘Chavez Dagostino Conference proceedings 2009 The Editor(s) (if applicabl

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The Chemical Composition of Elliptical Galaxies Through Mid-UV Indices,ide. On the basis of the Index vs [Fe/H] correlations seen in a sample of galactic globular clusters, we derived the chemical composition for all our sample galaxies. All resulting abundances are subsolar with Mg features delivering, on average, the lowest values.

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The Rest-Frame UV Spectrum of Elliptical Galaxies at High Redshift,a characteristic structure due to a set of iron and magnesium lines lines at λ≃eq 2600–2850 Å in the rest frame. The same feature permits also to estimate the time elapsed since the cessation of star formation. Current efforts at observing high redshift PEGs at the VLT and SUBARU telescopes are brie

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Rest-Frame UV and Visible Properties of Early Type Galaxies at 1 < , < 2,vely evolving systems provide constraints on the formation redshift and abundances for the oldest stars at a time when the universe was roughly 1/3 its present age. The passive galaxies have spectra characteristic of F stars with strong absorption from MgII, MgI and FeII. Best fitting ages are in th

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,Near UV Properties of Early–Type Galaxies at z ~ 1,ype Galaxies (ETG) at 0.88

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