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/

  • Very small grain emission in NGC 7023.
    We observed the reflection nebula NGC 7023 at various positions using wide and narrow band photometry centred on the 7.7 and 11.3μm PAH emission features and wide band photometry at 20 and 25μm. No significant variations have been detected over the nebula in the 7.3 and 20μm continuum relative to the total emission in the 6-15μm range (hereafter
    Laureijs, R. J. et al.

    Advertised on:

    11
    1996
    Citations
    13
  • VI and [Fe/H] of Fornax dSph RGB stars (Battaglia+, 2006)
    We present the results of the DART imaging and CaII triplet (CaT) survey of the Fornax dwarf spheroidal galaxy (dSph) at ESO. We collected hundreds of low resolution spectra of Red Giant Branch (RGB) stars in the CaT region, using VLT/FLAMES in Medusa mode, with the GIRAFFE spectrograph (grating LR8, resolving power R~6500). We list the results for
    Battaglia, G. et al.

    Advertised on:

    11
    2006
    Citations
    0
  • VII Zw403 - a BCD galaxy with an X-ray emission excess.
    VII Zw403 is a nearest BCD galaxy. This izolated system is so close (~4.5 Mp c), that it makes it possible to study it's star forming regions with unprecedently great details. recent X-ray observations (Papaderos et al. 1994) added more interest to the system, as revealed an extended, kpc-scale region of the diffuse X-ray emission. We use our
    Silich, S. et al.

    Advertised on:

    11
    2000
    Citations
    0
  • VIRGO: The solar monitor experiment on SOHO
    The Variability of solar IRradiance and Gravity Oscillations (VIRGO) experiment contains two types of active cavity radiometers for monitoring of the solar constant, two three channel sunphotometers for the measurement of spectral irradiance at 335, 500 and 865 nm and a low resolution imager with 12 pixels. The main scientific objective is probing
    Froehlich, C. et al.

    Advertised on:

    11
    1988
    Citations
    0
  • Visible and near-infrared spectroscopic survey of Jupiter Trojan asteroids: investigation of dynamical families
    Trojan asteroids located in the Jupiter Lagrangian points L4 and L5 (60 degrees ahead and behind Jupiter) are widely believed to be primordial bodies since their orbits are stable over the age of the Solar System. They seem to have been formed in a region of the solar nebula rich in frozen volatiles and to have never suffered selective induction
    Dotto, E. et al.

    Advertised on:

    11
    2004
    Citations
    0
  • Volatiles and refratories in solar analogs: No terrestial planet connection
    We have analysed very high-quality HARPS and UVES spectra of 95 solar analogs, 24 hosting planets and 71 without detected planets, to search for any possible signature of terrestial planets in the chemical abundances of volatile and refractory elements with respect to the solar abundances. We demonstrate that stars with and without planets in this
    González Hernández, J. I. et al.

    Advertised on:

    11
    2011
    Citations
    6