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/

  • X-ray Binaries in the Nearby Starburst Galaxy IC 10: A New Lab for Astrophysics
    We present early results of our Chandra study of transient X-ray binaries (XRB) in IC 10, the youngest and most active starburst galaxy in the local universe. X-ray binaries containing black-holes and neutron stars are the relics of the most massive, short-lived stars, and are highly visible tracers of star formation. Visible at intergalactic
    Laycock, Silas et al.

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    1
    2010
    Citations
    1
  • Washington photometry of five star clusters in the Large Magellanic Cloud
    We present CCD photometry in the Washington-system C and T1 passbands down to T1 ~ 22.5 mag in the fields of NGC 1697, SL 133, NGC 1997, SL 663, and OHSC 28, five mostly unstudied star clusters in the LMC. Cluster radii were estimated from star counts in appropriately sized boxes distributed throughout the entire observed fields. We perform a
    Piatti, Andrés E. et al.

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    1
    2010
    Citations
    0
  • UBV(RI)C photometry of the open clusters Be 15, Be 80 and NGC 2192
    The three open clusters Be 15, Be 80 and NGC 2192 have been observed using CCD UBV(RI)C photometry at the San Pedro Mártir Observatory, México within the framework of our open-cluster survey. The fundamental parameters of interstellar reddening, distance and age have been derived, and also the metallicity for NGC 2192 (solar metallicity has been
    Tapia, M. T. et al.

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    1
    2010
    Citations
    12
  • Type I X-ray bursts, burst oscillations and kHz quasi-periodic oscillations in the neutron star system IGRJ17191-2821
    We present a detailed study of the X-ray energy and power spectral properties of the neutron star transient IGRJ17191-2821. We discovered four instances of pairs of simultaneous kilohertz quasi-periodic oscillations (kHz QPOs). The frequency difference between these kHz QPOs is between 315 and 362Hz. We also report on the detection of five
    Altamirano, D. et al.

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    1
    2010
    Citations
    27
  • The VLT-FLAMES Tarantula Survey
    The Tarantula Survey is an ambitious ESO Large Programme that has obtained multi-epoch spectroscopy of over 1000 massive stars in the 30 Doradus region in the Large Magellanic Cloud. Here, we introduce the scientific motivations of the survey and give an overview of the observational sample. Ultimately, quantitative analysis of every star, paying
    Evans, C. J. et al.

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    1
    2010
    Citations
    23
  • The Role of Vesc in Early Type Galaxy Evolution
    How the stellar mass of early-type galaxies is assembled remains an open question. Are the stars formed in situ, possibly triggered by merger events, or do they form in smaller systems before being added to the host galaxy through mergers? Using the SAURON sample of local early-type galaxies combined with dynamical modelling we searched for
    Scott, Nicholas et al.

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    1
    2010
    Citations
    0