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/

  • Long-Term Trends and Gleissberg Cycles in Aurora Borealis Records (1600 - 2015)
    The long-term spatial and temporal variation of aurora borealis events from 1600 to the present were studied using catalogues and other records of these phenomena. Geographic and geomagnetic coordinates were assigned to approximately 45 000 auroral events with more than 160 000 observations. They were analysed separately for three large-scale areas
    Vázquez, M. et al.

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    2
    2016
    Citations
    28
  • KIC 9246715: The Double Red Giant Eclipsing Binary with Odd Oscillations
    We combine Kepler photometry with ground-based spectra to present a comprehensive dynamical model of the double red giant eclipsing binary KIC 9246715. While the two stars are very similar in mass ({M}1={2.171}-0.008+0.006 {M}ȯ , {M}2={2.149}-0.008+0.006 {M}ȯ ) and radius ({R}1={8.37}-0.07+0.03 {R}ȯ , {R}2={8.30}-0.03+0.04 {R}ȯ ), an asteroseismic
    Rawls, M. L. et al.

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    2
    2016
    Citations
    42
  • Impact of surface dynamo magnetic fields on the solar abundance of the CNO elements
    Most studies of the solar metallicity, based on abundance determinations of the CNO elements, ignore the fact that the quiet solar photosphere is significantly magnetized by a small-scale magnetic field with a mean field strength of ~100 G. Here we quantify how this significant magnetization affects determinations of the abundances of these
    Shchukina, N. et al.

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    2
    2016
    Citations
    12
  • High-speed Photometry of the Disintegrating Planetesimals at WD1145+017: Evidence for Rapid Dynamical Evolution
    We obtained high-speed photometry of the disintegrating planetesimals orbiting the white dwarf WD 1145+017, spanning a period of four weeks. The light curves show a dramatic evolution of the system since the first observations obtained about seven months ago. Multiple transit events are detected in every light curve, which have varying durations (
    Gänsicke, B. T. et al.

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    2
    2016
    Citations
    103
  • Globular Cluster Populations: Results Including S4G Late-type Galaxies
    Using 3.6 and 4.5 μm images of 73 late-type, edge-on galaxies from the S4G survey, we compare the richness of the globular cluster populations of these galaxies to those of early-type galaxies that we measured previously. In general, the galaxies presented here fill in the distribution for galaxies with lower stellar mass, M*, specifically {log}({M
    Zaritsky, D. et al.

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    2
    2016
    Citations
    8
  • Fossil group origins. VII. Galaxy substructures in fossil systems
    Context. Fossil groups (FG) are expected to be the final product of galaxy merging within galaxy groups. In simulations, they are predicted to assemble their mass at high redshift. This early formation allows for the innermost M∗ galaxies to merge into a massive central galaxy. Then, they are expected to maintain their fossil status because of the
    Zarattini, S. et al.

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    2
    2016
    Citations
    19