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/

  • Discovery of a planetary nebula surrounding the symbiotic star DT Serpentis

    We report the discovery of a planetary nebula centered on the poorly studied symbiotic binary star DT Ser. In a few other symbiotic stars spatially resolved nebulae have been discovered as well, but only one of them probably is a genuine planetary nebula, while the others are likely to originate in complex mass-ejection episodes from the

    Munari, U. et al.

    Advertised on:

    10
    2013
    Citations
    5
  • Discovery of a very cool object with extraordinarily strong Hmathsf α emission

    We report on the finding of the strongest Hα emission - pseudoequivalent width of 705 Å- known so far in a young, late type dwarf. This object, named as S Ori 71, is a substellar candidate member of the 1-8 Myr star cluster sigma Orionis. Due to its overluminous location in color-magnitude diagrams, S Ori 71 might be younger than other cluster

    Barrado y Navascués, D. et al.

    Advertised on:

    10
    2002
    Citations
    43
  • Discovery of mHz QPOs and burst rate evolution in the active Terzan 5 neutron star transient

    We report on RXTE observations of the neutron star transient currently active in Terzan 5 (also known as IGR J17480-2446; ATels #2919, #2920, #2922, #2924, #2929, #2932, #2933, #2937, #2939, #2940, #2946), which has recently turned into a Z source (Altamirano et al., ATel #2952). The X-ray burst rate has increased gradually (see also ATels #2939,

    Linares, M. et al.

    Advertised on:

    10
    2010
    Citations
    18
  • Discovery of the Broad-lined Type Ic SN 2013cq Associated with the Very Energetic GRB 130427A

    Long-duration gamma-ray bursts (GRBs) at z < 1 are found in most cases to be accompanied by bright, broad-lined Type Ic supernovae (SNe Ic-BL). The highest-energy GRBs are mostly located at higher redshifts, where the associated SNe are hard to detect observationally. Here, we present early and late observations of the optical counterpart of the

    de Ugarte Postigo, A. et al.

    Advertised on:

    10
    2013
    Citations
    113
  • Discovery of the Massive Overcontact Binary VFTS352: Evidence for Enhanced Internal Mixing

    The contact phase expected to precede the coalescence of two massive stars is poorly characterized due to the paucity of observational constraints. Here we report on the discovery of VFTS 352, an O-type binary in the 30 Doradus region, as the most massive and earliest spectral type overcontact system known to date. We derived the 3D geometry of the

    Almeida, L. A. et al.

    Advertised on:

    10
    2015
    Citations
    52
  • Discovery of the Near-infrared Counterpart to the Luminous Neutron-star Low-mass X-Ray Binary GX 3+1

    Using the High Resolution Camera on board the Chandra X-ray Observatory, we have measured an accurate position for the bright persistent neutron star X-ray binary and atoll source GX 3+1. At a location that is consistent with this new position, we have discovered the near-infrared (NIR) counterpart to GX 3+1 in images taken with the PANIC and

    van den Berg, Maureen et al.

    Advertised on:

    10
    2014
    Citations
    12