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: LIRIS (red dots) and NIRSPEC (black line) spectra of Pleiades proper motion candidates. The NIRSPEC spectrum of Calar 21 is normalized to the K-band LIRIS spectrum. The left panel illustrates the comparison of the Pleiades data with field,
    We report on the near-infrared low-resolution spectroscopy and red optical (Z-band) photometry of seven proper-motion, very low-mass substellar member candidates of the Pleiades cluster with magnitudes in the interval J=17.5-20.8 and K=16.1-18.5 mag. Spectra were acquired for six objects with the LIRIS and NIRSPEC instruments mounted on the 4.2-m WHT and the 10-m Keck II telescopes. Z-band images of two of the faintest candidates were collected with ACAM/WHT. The new data confirm the low temperatures of all seven Pleiades candidates. From the imaging observations, we find extremely red Z-J
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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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