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Rotational broadening and Doppler tomography of the quiescent X-ray nova Centaurus X-4
Authors:M A P Torres  J Casares  I G Martínez-Pais  P A Charles
Institution:Instituto de Astronomía y Fisica del Espacio, CC 67, Suc. 28, 1428, Capital Federal, Argentina;Universidade Federal do Rio Grande do Sul, Departmento de Astronomía, CP 15051, Porto Alegre, 91500-970, Brazil;Observatorio Astronómico, Laprida 854, 5000 Córdoba, Argentina;Departamento de Física, ICEx, UFMG, CP 702, 30123-970 Belo Horizonte, MG, Brazil
Abstract:We present a library of 47 open-cluster integrated spectra, mostly obtained at CASLEO (San Juan, Argentina) in the range  3600 < λ < 7400 Å  , which are made available at CDS. The data are combined with previous spectra to obtain 10 high signal-to-noise ratio basic templates in the young and intermediate-age domains, which are also provided in the library. These Galactic disc templates represent the increased time resolution spectral evolution of a stellar population unit around the Solar metallicity level. The improved signal-to-noise ratio of the present templates with respect to previous template lists, together with their increased time resolution, allowed us to improve the fundamental parameters of some open clusters. The present spectral library will be useful for several astrophysical applications, particularly for population syntheses of star-forming giant galaxies.
Keywords:techniques: spectroscopic  open cluster and associations: general  galaxies: individual: Milky Way  galaxies: star clusters
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