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/

  • LA ESCALA DE TEMPERATURAS EFECTIVAS DE LAS ESTRELLAS DE LA BAJA SECUENCIA PRINCIPAL (TIPOS ESPECTRALES F0-K5)
    ESTA TESIS DOCTORAL CONTIENE LOS RESULTADOS DE UN PROGRAMA DE INVESTIGACION EN EL QUE SE HAN DETERMINADO EMPIRICAMENTE LAS RELACIONES TEMPERATURA EFECTIVA-COLOR-METALICIDAD PARA ESTRELLAS DE SECUENCIA PRINCIPAL CON TIPOS ESPECTRALES COMPRENDIDOS EN EL RANGO F0-K5. PARA LLEVAR A CABO ESTA CALIBRACION HA SIDO NECESARIO DESARROLLAR UNA SERIE DE
    ANGEL ALONSO SANCHEZ

    Advertised on:

    5
    1995
  • ON THE RELATIONSHIP BETWEEN STAR FORMATION AND ACTIVITY IN GALAXIES
    EL OBJETO DE ESTA MEMORIA ES EL ESTUDIO DE LA RELACION ENTRE LOS PROCESOS DE FORMACION ESTELAR Y LA ACTIVIDAD EN EL NUCLEO DE LAS GALAXIAS. CON ESTE FIN SE ESTUDIA, EN PRIMER LUGAR, LA FORMACION ESTELAR EN LAS GALAXIAS ANALIZANDO ESTADISTICAMENTE MAS DE 500 REGIONES HII EN 55 GALAXIAS. A PARTIR DE ESTOS DATOS SE DETERMINAN FUNCIONES DE LUMINOSIDAD
    ROSA MARIA GONZALEZ DELGADO

    Advertised on:

    5
    1995
  • Near-quiescent photometry of the X-ray transient J0422+32
    We present I-band photometry of the soft X-ray transient (SXT) J0422+32 taken during a low-brightness state over two weeks in 1993 October. The object had a mean V magnitude of 19.9, approximately 2mag above its subsequent, presumably quiescent, level of V~22.4. These data revealed a periodicity at 16.18h (significance level>99 per cent), but we
    Martin, A. C. et al.

    Advertised on:

    5
    1995
    Citations
    11
  • Determination of bolometric fluxes for F, G and K subdwarfs
    Bolometric fluxes for 118 dwarfs and subdwarfs with 4000K less than Teff less than 7000K and +0.5 less than (Fe/H) less than -3.5 are derived by integrating UBVRIJHK photometry. For these stars (typical of the galactic and globular cluster main sequences) at least 80% of the energy emitted is measured by those bands. A grid of theoretical model
    Alonso, A. et al.

    Advertised on:

    5
    1995
    Citations
    156
  • Galactic evolution of beryllium. I. NLTE effects and accuracy of beryllium abundances in metal-poor stars.
    We have investigated in detail the uncertainties in deriving beryllium abundances for metal-poor stars from the BeII resonance doublet at λ 3131A. These uncertainties are related to the quality of the observations, the physical data used, and the adopted stellar parameters. We have taken into account the NLTE effects on the lines formation for the
    Garcia Lopez, R. J. et al.

    Advertised on:

    5
    1995
    Citations
    43
  • Electromagnetic force and geometry of Minkowskian spacetime
    By describing the dynamical evolution of a test charged particle in the presence of an electromagnetic field and a succession of infinitesimal Lorentz boosts and rotations it is possible to obtain the Lorentz force of electrodynamics. A consequence of this heuristic derivation at the classical level is that, given the existence of electric and
    Buitrago, J.

    Advertised on:

    5
    1995
    Citations
    1