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/

  • The Universidad Complutense of Madrid meteor and fireball patrol station
    The Universidad Complutense of Madrid (UCM) has recently installed a high sensitivity video system to detect meteors. It is intended to study the entry in our atmosphere of interplanetary particles of mass greater than a gram. The station, not fully equipped yet, is a node of the national Spanish Fireball Network (SPMN) and includes cameras located
    Zamorano, J. et al.

    Advertised on:

    11
    2011
    Citations
    0
  • The Unrelaxed Dynamical Structure of the Galaxy Cluster Abell 85
    For the first time, we explore the dynamics of the central region of a galaxy cluster within r 500 ∼ 600 h‑1 kpc from its center by combining optical and X-ray spectroscopy. We use (1) the caustic technique, which identifies the cluster substructures and their galaxy members with optical spectroscopic data, and (2) the X-ray redshift fitting
    Tozzi, P. et al.

    Advertised on:

    11
    2016
    Citations
    22
  • The use of turbulence-profile measurements to predict the performance of adaptive optics systems
    It is planned to include adaptive optics as an integral part of the 10-m Gran Telescopio Canarias. Preliminary scientific requirements have been drawn up, and it is necessary to identify systems which will satisfy these requirements. The approach adopted here is to use the LACE program to model the adaptive-optics system. The program provides for
    Devaney, N. et al.

    Advertised on:

    11
    1998
    Citations
    1
  • The variable mass loss of the peculiar supergiant P Cygni.
    The study of iron lines from 49 high-resolution IUE spectra observed in the period of 1985-1991 allowed us to find a repetition time between two successive shells of the order of six months. We found that absorption lines of Fe III often have two components while Fe II lines can have three. P Cygni is the only luminous blue variable that does not
    Israelian, G. et al.

    Advertised on:

    11
    1996
    Citations
    15
  • The Variable Radio-to-X-Ray Spectrum of the Magnetar XTE J1810-197
    We have observed the 5.54 s anomalous X-ray pulsar XTE J1810-197 at radio, millimeter, and infrared (IR) wavelengths, with the aim of learning about its broadband spectrum. At the IRAM 30 m telescope, we have detected the magnetar at ν=88 and 144 GHz, the highest radio-frequency emission ever seen from a pulsar. At 88 GHz we detected numerous
    Camilo, F. et al.

    Advertised on:

    11
    2007
    Citations
    86
  • The visible spectrum of Pluto: secular and longitudinal variation
    Continuous near-infrared spectroscopic observations during the last 30 years enabled the characterization of the Pluto's surface and the study of its variability. Nevertheless, only few data are available in the visible range, where the nature of the complex-organics can be studied.For this reason, we started an observational campaign to obtain the
    Lorenzi, V. et al.

    Advertised on:

    11
    2015
    Citations
    0