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
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Magnetic bright points in the quiet SunNot AvailableSánchez-Almeida, J. et al.
Fecha de publicación:
52010 -
Magnetic Bright Points in the Quiet SunWe present a visual determination of the number of bright points (BPs) existing in the quiet Sun, which are structures though to trace intense kG magnetic concentrations. The measurement is based on a 0farcs1 angular resolution G-band movie obtained with the Swedish Solar Telescope at the solar disk center. We find 0.97 BPs Mm-2, which is a factorSánchez-Almeida, J. et al.
Fecha de publicación:
52010 -
Infrared Imaging And SEDs With Spitzer Of Luminous Compact Blue Galaxies At z<1We present new infrared images and photometry with Spitzer/IRAC + MIPS of over 20 luminous compact blue galaxies (LCBGs), half at z 0 and half at z 0.75. LCBGs are extreme starburst galaxies with strong evolution, providing up to 40% of the observed increase in global star formation rate density between z=0 and z=1. They are important to study asLowenthal, James D. et al.
Fecha de publicación:
52010 -
Impact of internal bremsstrahlung on the detection of γ rays from neutralinosWe present a detailed study of the effect of internal bremsstrahlung photons in the context of the minimal supersymmetric standard models and their impact on γ-ray dark matter annihilation searches. We find that, although this effect has to be included for the correct evaluation of fluxes of high energy photons from neutralino annihilation, itsCannoni, M. et al.
Fecha de publicación:
52010 -
Formation of a multi-thread prominenceSolar prominences are composed of many threads of cool and dense plasma suspended in the million-degree solar corona. We have constructed a 3D time-dependent model of a prominence from 1D independent simulations of many flux tubes. The 3D magnetic field is taken from an adaptive MHD simulation of a sheared double-arcade filament channel. We willLuna Bennasar, Manuel et al.
Fecha de publicación:
52010