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/

  • Lithium in black hole binaries: the case of X-ray Nova Muscae 19911
    We report the detection of the LiI λ6708 resonance line in the K4V secondary of the black-hole binary Nova Muscae 1991. The LiI feature changes with orbital phase, being stronger (EW ∼ 400 mÅ) around φ = 0.0 (observing the dark side of the secondary) and weaker (EW ≤ 190 mÅ) around φ = 0.5 (observing the side facing the compact object). This effect
    Martin, E. L. et al.

    Advertised on:

    11
    1996
    Citations
    32
  • ISOPHOT - capabilities and performance.
    ISOPHOT covers the largest wavelength range on ISO from 2.5 to 240μm. Its scientific capabilities include multi-filter and multi-aperture photometry, polarimetry, imaging and spectrophotometry. All modes can optionally include a focal plane chopper. The backbone of the photometric calibration are internal standard sources checked against celestial
    Lemke, D. et al.

    Advertised on:

    11
    1996
    Citations
    489
  • H II REGIONS IN THE DISCS OF SPIRAL GALAXIES.FECHA DE LA DEFENSA
    EN LA PRIMERA PARTE DE ESTA TESIS SE PRESENTA UNA CATALOGACION Y ANALISIS ESTADISTICO DE LAS REGIONES H II DE VARIAS GALAXIAS ESPIRALES DE GRAN DISEÑO, DE LAS QUE SE HAN OBTENIDO IMAGENES DE CALIDAD FOTOMETRICA Y GRAN RESOLUCION ANGULAR: POSICIONES, TAMAÑOS, FLUJOS, ETC. EL ANALISIS DE ESTAS PROPIEDADES HA DADO LUGAR AL DESCUBRIMIENTO DE UNA
    MAITE ROZAS ESPADAS

    Advertised on:

    11
    1996
  • Global morphology and physical relations between the stars, gas and dust in the disc and arms of M100.
    We study star formation processes in the disc of the weakly barred grand design spiral galaxy M100 (NGC 4321) from a variety of images tracing recent massive star formation, old and young stars, dust and neutral hydrogen. Differences between arm and interarm regions are specifically studied by decomposing the images into arm and non-arm zones. We
    Knapen, J. H. et al.

    Advertised on:

    11
    1996
    Citations
    40