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
    A spectroscopic analysis of the Trapezium Cluster stars
    We consider the Orion Nebula (M 42) within a project aimed at studying the interaction between massive stars and their surrounding ISM. This is an HII region ionized by θ1 Ori C, one of the four massive stars in the Trapezium Cluster. θ1 Ori C has the earliest spectral type (O7Vp) among them, emitting an ionizing flux several orders of magnitude
    Simón-Díaz, Sergio et al.

    Advertised on:

    0
    2003
    Bibcode
    2003IAUS..212..749S
    Citations
    0
  • Non-refereed
    A spectral atlas of Landolt stars for a reliable mid-IR spectrophotometric calibration for large telescopes
    It is often stated that there is no point in obtaining mid-infrared data with S/N>20, even in the best of cases, because it is impossible to obtain a calibration to better than 5%, although in many cases 10% or greater is a more accurate reflection of the true quality of calibration. Mid-infrared calibration is difficult because of the lack of
    Martín-Luis, F. et al.

    Advertised on:

    0
    2003
    Bibcode
    2003RMxAC..16..296M
    Citations
    0
  • Non-refereed
    A numerical laboratory for the diagnostics of stellar properties
    In a recent paper (Crivellari et al., 2003) we summarized the principles of the algorithmic representation of the structure of a stellar atmosphere. We mentioned there our recent progresses in the numerical treatment of both the global method and the basic components of the corresponding models. As the natural sequel to that paper, we wish to
    Crivellari, L. et al.

    Advertised on:

    0
    2003
    Bibcode
    2003MSAIS...3...97C
    Citations
    2
  • Non-refereed
    A New Scenario for the Formation of Massive Stellar Clusters
    A new scenario is proposed in which the continuous creation of stars results into a highly concentrated massive (globular cluster-like) stellar system. We show that under very general conditions a large-scale gravitational instability in the ISM that triggers the collapse of a massive cloud leads with the aid of newly-formed stars to a standing
    Palous, Jan et al.

    Advertised on:

    0
    2003
    Bibcode
    2003IAUJD..11E..24P
    Citations
    0