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

  • Sin árbitro
    Merging Clusters of DARC Sample: studying the simultaneous formation of galaxy systems and their brightest galaxies
    Not Available
    Girardi, Marisa et al.

    Fecha de publicación:

    6
    2011
    Bibcode
    2011fvc..confP..17G
    Número de citas
    0
  • Sin árbitro
    MASTER Bright Flare 163942.75 +122414.4 discovery
    The MASTER auto-detection system at Tunka (Baykal Lake) detected a new transient source at the position (R.A., Dec) = 16h 39m 42.75s, +12d 24m 14s.4, (J2000) with a typical uncertainty of 0.5" at 2011-06-04 18:34:49.39 (UT). The OT is seen at 2 images. There is CV type star inside error box B2=20.14 and R2=20.23 (USNOB). The unfiltered (0.2B+0.8R)
    Balanutsa, P. et al.

    Fecha de publicación:

    6
    2011
    Bibcode
    2011ATel.3427....1B
    Número de citas
    1
  • Sin árbitro
    Mass function of IC4665 from UKIDSS-GCS (Lodieu+, 2011)
    Knowledge of the mass function in open clusters constitutes one way to constrain the formation of low-mass stars and brown dwarfs along with the knowledge of the frequency of multiple systems and the properties of disks. The aim of the project is to determine the shape of the mass function in the low-mass and substellar regimes in the pre-main
    Lodieu, N. et al.

    Fecha de publicación:

    6
    2011
    Bibcode
    2011yCat..35329103L
    Número de citas
    0
  • Con árbitro
    Magnetohydrodynamic turbulent cascade of coronal loop magnetic fields
    The Parker model for coronal heating is investigated through a high resolution simulation. An inertial range is resolved where fluctuating magnetic energy EM(k⊥)∝k⊥-2.7 exceeds kinetic energy EK(k⊥)∝k⊥-0.6. Increments scale as δbℓ≃ℓ-0.85andδuℓ≃ℓ+0.2 with velocity increasing at small scales, indicating that magnetic reconnection plays a prime role
    Rappazzo, A. F. et al.

    Fecha de publicación:

    6
    2011
    Bibcode
    2011PhRvE..83f5401R
    Número de citas
    24