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/

  • Non-refereed
    Extrasolar planets and Their Parent Stars
    Extrasolar planetas (exoplanets), or planets orbiting stars other than our own Sun, are a relatively new field of the astronomical and planetary sciences. After the discovery of Pluto in 1930, planet-finding activities appeared to have reached an end for the foreseeable future. Several brown dwarfs have been discovered between 1930 and 1993
    Israelian, G.

    Advertised on:

    11
    2010
    Bibcode
    2010vaoa.conf..318I
    Citations
    1
  • Refereed
    Evolution of dust temperature of galaxies through cosmic time as seen by Herschel
    We study the dust properties of galaxies in the redshift range 0.1 ~ 5 × 1010Lsolar appears to be 2-5K colder than that of AKARI-selected local galaxies with similar luminosities, and the dispersion in Tdust for high-z galaxies increases with LIR due to the existence of cold galaxies that are not seen among local galaxies. We show that this large
    Hwang, H. S. et al.

    Advertised on:

    11
    2010
    Bibcode
    2010MNRAS.409...75H
    Citations
    156
  • Non-refereed
    Early-type galaxies in the EGS (Fernandez Lorenzo+, 2011)
    Physical parameters for 135 early-type galaxies in the Extended Groth Strip (EGS). For each galaxy equatorial coordinates, total magnitudes in B and g-bands, redshift, velocity dispersion, effective radius, surface brightness, stellar mass, Sersic index, type (elliptical or lenticular) and signal-to-noise of the spectrum are given. (1 data file).
    Fernandez Lorenzo, M. et al.

    Advertised on:

    11
    2010
    Bibcode
    2010yCat..35269072F
    Citations
    0
  • Non-refereed
    Dynamical masses for the nearest brown dwarf binary: ɛ Indi Ba,b
    Binary brown dwarfs are important because their dynamical masses can be determined in a model-independent way. If a main sequence star is also involved, the age and metallicity for the system can be determined, making it possible to break the sub-stellar mass-age degeneracy. The most suitable benchmark system for intermediate age T dwarfs is ɛ Indi
    Cardoso, C. V. et al.

    Advertised on:

    11
    2010
    Bibcode
    2010HiA....15..761C
    Citations
    2