Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Chemical abundance of 12 stars in open clusters (Carrera+, 2011)

    Using high-resolution (R~30000), high-quality (S/N>=60 per pixel), we obtained spectra for twelve stars in four open clusters with the fibre spectrograph FOCES, at the 2.2 Calar Alto Telescope in Spain.We employ a classical equivalent-width analysis to obtain accurate abundances of sixteen elements: Al, Ba, Ca, Co, Cr, Fe, La,Mg, Na, Nd, Ni, Sc, Si

    Carrera, R. et al.

    Advertised on:

    9
    2011
    Citations
    0
  • Chemical Abundances and Kinematics of the Ring Nebula and Its Halos

    We have obtained new narrowband CCD images, spatially resolved intermediate- and high-dispersion spectroscopic observations of the Ring Nebula (NGC 6720). These data reveal that the bright main nebula is not a real ring, but a closed shell. A prolate ellipsoidal geometry for this shell is inferred from the observed tilts in the [N II] velocity

    Guerrero, M. A. et al.

    Advertised on:

    9
    1997
    Citations
    38
  • Chemical abundances and masses of the haloes around the planetary nebulae NGC 6543 and NGC 6826

    Spatial resolved low resolution spectroscopy of the haloes around the planetary nebulae NGC 6543 and NGC 6826 were conducted. The results imply that the radiation is thermal and not due to dust reflection. From those data chemical abundances and masses were calculated. Chemical abundances decrease in the haloes, while masses increase up to ten

    Manchado, A. et al.

    Advertised on:

    9
    1989
    Citations
    40
  • Chemical Abundances from Inversions of Stellar Spectra: Analysis of Solar-Type Stars with Homogeneous and Static Model Atmospheres

    Spectra of late-type stars are usually analyzed with static model atmospheres in local thermodynamic equilibrium (LTE) and a homogeneous plane-parallel or spherically symmetric geometry. The energy balance requires particular attention, as two elements that are particularly difficult to model play an important role: line blanketing and convection

    Allende Prieto, Carlos et al.

    Advertised on:

    9
    2001
    Citations
    43
  • Chemical Abundances in the Secondary Star of the Neutron Star Binary Centaurus X-4

    Using a high-resolution spectrum of the secondary star in the neutron star binary Cen X-4, we have derived the stellar parameters and veiling caused by the accretion disk in a consistent way. We have used a χ2 minimization procedure to explore a grid of 1,500,000 LTE synthetic spectra computed for a plausible range of both stellar and veiling

    González Hernández, Jonay I. et al.

    Advertised on:

    9
    2005
    Citations
    27
  • Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program. Galactic stellar populations and planets

    Context. We performed a uniform and detailed abundance analysis of 12 refractory elements (Na, Mg, Al, Si, Ca, Ti, Cr, Ni, Co, Sc, Mn, and V) for a sample of 1111 FGK dwarf stars from the HARPS GTO planet search program. Of these stars, 109 are known to harbor giant planetary companions and 26 stars are exclusively hosting Neptunians and super

    Adibekyan, V. Zh. et al.

    Advertised on:

    9
    2012
    Citations
    473