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/

  • Forces on magnetic flux tubes moving in inhomogeneous flows
    The back-reaction of an incompressible two-dimensional flow of constant strain to the accelerated motion of a straight cylinder is calculated in the general case that the flow is inhomogeneous, nonstationary, and with nonvanishing (although constant) vorticity. The resulting enhanced inertia of the cylinder is basically given by its relative
    Moreno-Insertis, F. et al.

    Advertised on:

    2
    1994
    Citations
    5
  • Early Evolution of Low Mass Stars and Objects Close to the Substellar Mass Limit
    The subject of this study is the pre-main sequence (PMS) evolution of stars less massive than ~1.2 solar mass, using lithium as the main tool for confronting model predictions with observations. In addition, it is proposed to use Li as a test of the possible substellar nature of brown dwarf candidates. The main results of this work are: 1.) The
    Martin, E. L.

    Advertised on:

    2
    1994
    Citations
    0
  • Dependence of the population index on the radiant zenithal distance
    By integrating the differential equation system of the single-body meteor theory which describes meteor flight in the atmosphere, we show that the population index r depends on the radiant zenithal distance zR. When zR is large, r diminishes, requiring correction in order to obtain reliable number density profiles. A new method is proposed to
    Bellot Rubio, L. R.

    Advertised on:

    2
    1994
    Citations
    4
  • A semi-empirical absolute flux calibration in the near infrared: Direct stellar diameters vs. IRFM determinations
    A new semi-empirical method to derive the absolute flux calibration in the near infrared (J,K,L and L' bands) is proposed. The method consists of the application of the InfraRed Flux Method (IRFM) to a selected sample of stars with accurate direst measurements of their angular diameters. The absolute fluxes in each band are obtained minimizing the
    Alonso, A. et al.

    Advertised on:

    2
    1994
    Citations
    49