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

  • An Asymptotic Solution for the Navier-Stokes Equation
    We have used as the velocity field of a fluid the functional form derived in Casuso (2007), obtained by studying the origin of turbulence as a consequence of a new description of the density distribution of matter as a modified discontinuous Dirichlet integral. Asan interesting result we have found that this functional form for velocities is a
    Beckman J. E. et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    0
  • An anticorrelation between X-ray luminosity and Hα equivalent width in X-ray binaries
    We report an anticorrelation between continuum luminosity and the equivalent width (EW) of the Hα emission line in X-ray binary systems. The effect is evident both in a universal monotonic increase in Hα EW with time following outbursts, as systems fade, and in a comparison between measured EWs and contemporaneous X-ray measurements. The effect is
    Fender, R. P. et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    25
  • A Planet in a 0.6 AU Orbit Around the K0 Giant HD 102272
    We report the discovery of one or more planet-mass companions to the K0-giant HD 102272 with the Hobby-Eberly Telescope. In the absence of any correlation of the observed periodicities with the standard indicators of stellar activity, the observed radial velocity variations are most plausibly explained in terms of a Keplerian motion of at least one
    Niedzielski, A. et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    69
  • A Novel Precise Method for Correcting the Temperature in Stellar Atmosphere Models
    A mayor problem that arises in the computation of stellar atmosphere models is the self consistent determination of the temperature distribution via the constraint of energy conservation. The energy balance includes the gains due to the absorption of radiation: int χ(ν) J(ν) dν, and the losses due to emission: int χ(ν) S(ν) dν . It is well known
    Cardona, O. et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    0
  • CARACTERIZACION MINERALOGICA DE ASTEROIDES CERCANOS A LA TIERRA
    Los asteroides son objetos que no poseen atmósfera cuyo tamaño es menor que el de los planetas y que orbitan alrededor del Sol. La principal población de estos objetos se encuentra entre las órbitas de Marte y Júpiter, en el denominado "cinturón principal" (main belt, MB). Dentro de los asteroides son de especial interés los asteroides cercanos a
    Julia Mª de León Cruz

    Fecha de publicación:

    3
    2009
  • ɛ Indi Ba, Bb: a spectroscopic study of the nearest known brown dwarfs
    The discovery of V Indi Ba and Bb, a nearby binary brown dwarf system with a main-sequence companion, allows a concerted campaign to characterise the physical parameters of two T dwarfs providing benchmarks against which atmospheric and evolutionary models can be tested. Some recent observations suggest the models at low mass and intermediate age
    King, Robert R. et al.

    Fecha de publicación:

    2
    2009
    Número de citas
    2