News

This section includes scientific and technological news from the IAC and its Observatories, as well as press releases on scientific and technological results, astronomical events, educational projects, outreach activities and institutional events.

  • Figure caption: Left panels show the i − J vs. g − r diagrams for three different parameters: surface brightness in restframe J (μJ, blue), the logarithm of the stellar mass density (log (ρ), pink), and the radial distance to the most massive galaxies of
    The ultra-deep multiwavelength Hubble Space Telescope Frontier Fields coverage of the Abell Cluster 2744 is used to derive the stellar population properties of its intracluster light (ICL). The restframe colors of the ICL of this intermediate redshift (z = 0.3064) massive cluster are bluer (g – r = 0.68 ± 0.04; i – J = 0.56 ± 0.01) than those found in the stellar populations of its main galaxy members (g – r = 0.83 ± 0.01; i – J = 0.75 ± 0.01). Based on these colors, we derive the following mean metallicity Z = 0.018 ± 0.007 for the ICL. The ICL age is 6 ± 3 Gyr younger than the average age
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  • Image of Messier 6, one of the galaxies in the study. Superposed dashed ellipses are rings indicating concentric density waves in this galaxy. Source: SLOAN + IACbia
    Astronomers at the IAC have discovered complex patterns of resonances in the discs of spiral galaxies not previously described by theories. Using the GHaFaS 2dimensional spectrometer they have measured the velocities of the density waves in the discs of over a hundred galaxies Within the discs of spiral galaxies there are waves which propagate concentrically in the form of spirals. This is somewhat similar to the waves on the surface of a lake, or the standing waves on the strings of a violin, or on the surface of a drum, to use a musical metaphor. These are the so-called “density waves”
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  • The galaxy NGC 1277 in the Perseus cluster. Copyright: Sloan Digital Sky Survey (SDSS).
    The nearby galaxy NGC 1277 was formed at an early epoch of the cosmos and has remainedunchanged since then, thus making it a unique window on to the early Universe. Astronomers have found that the rate of star formation in massive galaxies at that remote epoch was much higher than expected with a thousand times more stars being generated than at present in the Milky Way. Further information: Spanish Press Release
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