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

  • How Hot are Hot Stars?: New Temperatures for mid-O types from FUSE data
    We analysed high resolution spectra of Galactic O-type stars from the far-UV to the optical. We combined spectra from the Far Ultraviolet Spectroscopic Explorer (FUSE) in the range 905-1187Å, IUE or HST archive spectra (1150-3300Å), and optical blue and Hα spectra from the La Palma INT. The spectra were analysed with line-blanketed, hydrodynamic
    Bianchi, L. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    1
  • High-resolution solar polarimetry with Sunrise
    Sunrise is a solar telescope with an aperture of 1 m, and is dedicated for spectropolarimetric measurements in the visible and the near UV. The total wavelength range is 200 to 1000 nm for narrowband imaging and diagnostic spectroscopy. Sunrise is planned as a stratospheric long-duration balloon mission with a first flight in 2006
    Schmidt, W. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    4
  • Global Hybrid Simulation of the Magnetopause Boundary Layer in Low- and High-Latitude Magnetic Reconnections
    A 2-D global hybrid simulation is carried out to study the structure of the dayside magnetopause in the noon-midnight meridian plane associated with magnetic reconnection. In the simulation the bow shock, magnetosheath, and magnetopause are formed self-consistently by supersonic solar wind passing the geomagnetic field. The reconnection events at
    Xie, H. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    0
  • Gas Dynamics and Star Formation in the Grand-Design Spiral NGC 5248
    We present a multi-wavelength study of the gas dynamics and star formation in the grand-design spiral galaxy NGC 5248, illustrating how coupled dynamical mechanisms can generate spiral structures from tens of kpc to hundreds of pc, drive disk evolution, and fuel star formation on progressively smaller scales. Although to date NGC 5248 has been
    Jogee, S. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    0
  • Fast MHD oscillations in prominence fine structures
    High-resolution observations suggest that quiescent solar prominences are made of small-scale fibrils stacked one after another in both the vertical and horizontal directions. These fibrils are interpreted as the cool, highermost part of much larger coronal loops which are rooted in the solar photosphere. On the other hand, there is some evidence
    Díaz, A. J. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    51
  • Evolution of active galactic nuclei broad-line region clouds: low- and high-ionization lines
    The formation of quasar broad-line region (BLR) clouds via thermal instability in the presence of Alfvén heating has been discussed by Gonçalves, Jatenco-Pereira & Opher. In particular, these studies showed the relevance of Alfvén heating in establishing the stability of BLR clouds in the intercloud medium. The present paper shows the results of
    Gonçalves, D. R. et al.

    Fecha de publicación:

    12
    2001
    Número de citas
    3