Minor Planet Observations [950 La Palma]
Not Available
Fitzsimmons, A. et al.
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2010
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/
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Measurements and Simulations of Regolith Surface Roughness Effects in XRFAnalyses of fluorescent soft X-ray spectra from planetary surfaces obtained by orbiting spacecraft use the intensities of elemental emission lines and their ratios to, e.g., determine the geochemistry of the surface of the target body. Historically, in the analyses it has been assumed that the planetary surfaces can be considered as homogeneous andNäränen, J. et al.
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Luminous buried AGNs and the AGN-starburst connections in the local UniverseNot AvailableImanishi, M.
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Low and High Temperature Infrared Spectroscopy of C60 and C70 FullerenesThe FT-IR spectra of the fullerenes C60 and C70 have been recorded in the temperature range between 523 K (+250 degrees C) and 93 K (-180 degrees C). As a general rule, it has been observed a shift of the infrared absorption bands toward higher frequencies at lower temperatures. As expected, at 93 K the infrared spectra appear better resolved withManchado, A. et al.
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Light elements in stars with exoplanetsLight elements are important tracers of the internal stellar structure and kinematics. Li and Be are both burned in the stellar interiors but Be requires much higher temperatures and thus we can expect to measure Be abundances in stars which have no detectable Li in their atmospheres. The study of these elements can give us information aboutDelgado Mena, E. et al.
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La Astrofísica promotora de desarrollo científico, cultural, tecnológico y económicoNot AvailableSánchez, F.
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