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
    Novae in M81: M81N 2010-06a, M81N 2010-06b, M81N 2010-06c, M81N 2010-06d
    CBET 2338 available at Central Bureau for Astronomical Telegrams.
    Hornoch, K. et al.

    Advertised on:

    6
    2010
    Bibcode
    2010CBET.2338....1H
    Citations
    0
  • Non-refereed
    New outburst of the accreting millisecond X-ray pulsar NGC 6440 X-2 and discovery of a strong 1 Hz modulation in the light-curve
    On June 11th, 2010, RXTE/PCA galactic bulge scan observations showed an increase in activity from the globular cluster NGC 6440. Two accreting millisecond X-ray pulsars (AMXPs) and 22 other X-ray binaries are known in NGC 6440 (see Pooley et al. 2002, ApJ 573, 184, Altarmirano et al. 2010, ApJL 712, 58, Altamirano et al. 2008, ApJL 674, 45 and
    Patruno, A. et al.

    Advertised on:

    6
    2010
    Bibcode
    2010ATel.2672....1P
    Citations
    5
  • Refereed
    New groups of planetary nebulae with peculiar dust chemistry towards the Galactic bulge
    Aims: We investigate Galactic bulge planetary nebulae without emission-line central stars for which peculiar infrared spectra have been obtained with the Spitzer Space Telescope, including the simultaneous signs of oxygen and carbon based dust. Three separate sub-groups can be defined characterized by the different chemical composition of the dust
    Górny, S. K. et al.

    Advertised on:

    6
    2010
    Bibcode
    2010A&A...516A..39G
    Citations
    17
  • Non-refereed
    Multi-Wavelength Characterization of the Outskirts of Spiral Galaxies
    We have explored late-type spiral galaxies with truncated radial surface brightness profiles. Based on the study of optical color profiles, [1] suggested that truncated (TYPE II) galaxies have a generally older stellar population in their outer regions: one observable consequence of this would be a strong dependence of the structural parameters of
    Bakos, Judit et al.

    Advertised on:

    6
    2010
    Bibcode
    2010AIPC.1240..287B
    Citations
    1
  • Thesis
    MORPHOLOGY AND PHYSICAL PROPERTIES OF STAR FORMATION IN SPIRAL GALAXIES
    SEBASTIEN COMERON LIMBOURG

    Advertised on:

    6
    2010