Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Studies of cosmic microwave background structure at Dec.=+40 deg - I. The performance of the Tenerife experiments
    The direct identification of structure in the cosmic microwave background (CMB) is a major objective of observational cosmology. We present a detailed discussion of observations of such structure detected on a 5 deg scale in the CMB using beam-switching radiometers at 10, 15 and 33 GHz sited in Tenerife. This long-term experiment has reached
    Davies, R. D. et al.

    Fecha de publicación:

    2
    1996
    Número de citas
    35
  • Stellar models with rotation: an exploratory application to pre-main sequence Lithium Depletion.
    Over the last 20 years, the surface abundance of Li has been derived for a significant number of low mass pre-main sequence (PMS) stars. Several works have pointed out the unexpected large Li spread for young stars of similar ages and masses. This spread still represents a challenge in our understanding of PMS stellar evolution. Almost in parallel
    Claret, A. et al.

    Fecha de publicación:

    2
    1996
    Número de citas
    90
  • STARS - Seismic Telescope for Astrophysical Research from Space. Report on the phase A study.
    STARS is an asteroseismology mission, which, through the acquisition of very accurate light curves, will detect oscillations in a wide variety of stars. This will allow, for the first time, the internal structure of stars of different age, composition and spectral type, to be studied directly, bringing the spectacular successes of helioseismology
    Badiali, M. et al.

    Fecha de publicación:

    2
    1996
    Número de citas
    8
  • Spatial source distribution of bulges from surface photometry: application to NGC 2841.
    We tackle here the problem of obtaining the spatial density of sources ρ in the bulge of a spiral galaxy using bidimensional surface photometry. V,R,I,Z CCD images, taken with the 4.2m William Herschel Telescope at seeing limit resolution (0.5"-1.1"), yield the photometric parameters for the galaxy NGC 2841. The necessary procedure prior to
    Varela, A. M. et al.

    Fecha de publicación:

    2
    1996
    Número de citas
    17
  • Response functions for the inversion of data from unresolved solar magnetic elements.
    By adopting the thin flux tube model as representative of spatially unresolved magnetic elements in the photosphere of the Sun, we identify an adequate set of parameters for the model and derive the corresponding response functions (RFs) which inform about the variation of the emergent Stokes spectrum when such parameters are perturbed. We
    Bellot Rubio, L. R. et al.

    Fecha de publicación:

    2
    1996
    Número de citas
    12
  • On the Storage of Magnetic Flux Tubes at the Base of the Solar Convection Zone
    The study of the storage of toroidal flux tubes at the base of the convection zone is of interest in connection with the operation of a solar αΩ-type dynamo. The natural equilibrium state for an isolated flux tube is that of neutral buoyancy (so that there is a mass flow along the tube in the direction of solar rotation); flux tubes in thermal
    Ferriz-Mas, Antonio

    Fecha de publicación:

    2
    1996
    Número de citas
    15