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Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..
Además ofrece acceso al repositorio de preprints del IAC: https://research.iac.es/preprints/l
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Frequencies of Solar p-Modes from GOLF and VIRGO-SPM (SOHO)Roca-Cortés, T. et al.121999
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Frequency shift of solar p-modes as seen by cross correlation analysis
Data obtained at the Observatorio del Teide (Tenerife) during the years 1978 to 1988 using a resonant scattering spectrophotometer, is analyzed to look for variations of the low degree p-mode frequencies along the solar cycle. The analysis based on the cross-correlation of power spectra suggests that the variation of its maximum correlation
Palle, Pere L. et al.Fecha de publicación:
121988 -
From CoRoT 102899501 to the Sun. A time evolution model of chromospheric activity on the main sequence
Aims: The present study reports measurements of the rotation period of a young solar analogue, estimates of its surface coverage by photospheric starspots and of its chromospheric activity level, and derivations of its evolutionary status. Detailed observations of many young solar-type stars, such as the one reported in the present paper, provide
Gondoin, P. et al.Fecha de publicación:
122012 -
From Deterministic to Probabilistic Population Synthesis (Why Synthesis Models are not what we thought they were, and how they can be much more than that)
For a number of reasons, the properties of integrated stellar populations are distributed. Traditional synthesis models usually return the mean value of such distribution, and a perfect fitting to observational data is sought for to infer the age and metallicity of observed stellar populations. We show here that, while this is correct on average
Luridiana, V. et al.Fecha de publicación:
122007 -
From Gas to Starburst and AGN
Although it is clear that the circumnuclear regions of galaxies are intimately related to their host galaxies, most directly through their bars, it remains unclear what exactly initiates and fuels nuclear stellar (starburst) and non-stellar (AGN) activity. Deviations from axisymmetry in the gravitational potential of a galaxy, set up by a bar or an
Knapen, J.Fecha de publicación:
122004 -
Ft-Ir Spectra of Fullerenes C76, C78 and C84 At Temperatures Comprised Between -180°C and +250°C
The FT-IR spectra of C76, C78 and C84 fullerenes were recorded in the temperature range comprised between -180°C and +250°C. The purpose of the work is to provide reference infrared spectra for searching higher fullerene homologues in space after the recent and successful discovery of C60 and C70 in a series of different astrophysical objects.
Iglesias-Groth, S. et al.Fecha de publicación:
122013