Absorption line indices in the UV I. Empirical and theoretical stellar population models

Astronomy and Astrophysics

Volumn 493, Issue 2, 2009, Pages 425-444

  Maraston, C ^a   Nieves Colmenarez L ^b   Bender, R ^b,c   Thomas, D ^a  

^a UNIVERSITY OF PORTSMOUTH   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c UNIVERSITY OF MUNICH   (Germany)

Author keywords

Galaxies: evolution; Galaxies: Magellanic Clouds; Galaxies: star clusters; Galaxies: stellar content

Indexed keywords

ABSORPTION; CLOUDS; COSMOLOGY; FUNCTIONS; POPULATION STATISTICS; PROBABILITY DENSITY FUNCTION; STARS;

ABSORPTION LINES; ANALYTICAL FUNCTIONS; COMPREHENSIVE STUDIES; EVOLUTIONARY POPULATIONS; FITTING FUNCTIONS; GALAXIES: EVOLUTION; GALAXIES: MAGELLANIC CLOUDS; GALAXIES: STAR CLUSTERS; GALAXIES: STELLAR CONTENT; GLOBULAR CLUSTERS; HIGH RESOLUTIONS; HIGH-REDSHIFT; LOW RESOLUTIONS; MAGELLANIC CLOUDS; METALLICITIES; METALLICITY; NEW INDICES; RED SHIFTS; SPECTRAL ENERGY DISTRIBUTIONS; SPECTRAL LIBRARIES; SPECTRAL REGIONS; STELLAR POPULATIONS; STELLAR SPECTRUM; SYNTHETIC SPECTRUMS; ULTRAVIOLET ABSORPTIONS; WAVELENGTH RANGES;

GALAXIES;

EID: 59049084434     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066907     Document Type: Article

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