Formation of fullerenes in hydrogen-rich environments.
Thanks to the NASA’s Spitzer Space Telescope, bucket loads of large carbon molecules, the so-called fullerenes (C 60), have been found around dying stars in the...
Fullerenes in the IC 348 star cluster of the Perseus molecular cloud
We present the detection of fullerenes C 60 and C 70 in the star-forming region IC 348 of the Perseus molecular cloud. Mid-IR vibrational transitions of C 60...
Galactic superwinds present a filament-like structure, with strong X ray emissions, which could not be explained until now. Using hydrodynamic calculations, it...
Galaxy fusion provides an explanation for asymmetrical stellar velocities in elliptical galaxies
Using the IAC's Beowulf group of computers and the National Supercomputing Centre's Mare Nostrum, an IAC team has simulated the process of galaxy fusion by...
The aim of the project is to contribute to the characterisation of the spectral energy distribution of the coolest brown dwarfs discovered to date, the Y dwarfs...
HADES RV Programme with HARPS-N at TNG. V. A super-Earth on the inner edge of the habitable zone of the nearby M-dwarf GJ 625
We report the discovery of a new super-Earth orbiting the nearby cool dwarf star GJ 625 in the inner edge of the habitable zone. This result has been achieved...
Accretion disc winds are observed in accreting black holes across the full range of masses. In stellar-mass black holes, X-ray winds have been recently...
Height Variation of the vector magnetic field in solar spicules
Proving the magnetic configuration of solar spicules has hitherto been difficult due to the lack of spatial resolution and image stability during off-limb...
HELIO AND ASTERO-SEISMOLOGY AND EXOPLANETS SEARCH.
La huella de los modos-g en el Sol. Gracias a las medidas realizadas por el instrumento GOLF a bordo del satélite SoHO de modo ininterrumpido a lo largo de los...