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dc.contributor.authorDuffard, René D.-
dc.contributor.authorLeón, Julia María de-
dc.contributor.authorLicandro, J.-
dc.contributor.authorLazzaro, D.-
dc.contributor.authorSerra-Ricart, M.-
dc.date.accessioned2009-09-16T11:07:00Z-
dc.date.available2009-09-16T11:07:00Z-
dc.date.issued2006-09-
dc.identifier.citationAstronomy and Astrophysics 456(2): 775-781 (2006)en_US
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/10261/16991-
dc.description7 pages.en_US
dc.description.abstract[Aims] We present reflectance spectra of three V-type Near-Earth Objects obtained at the 3.6 m Telescopio Nazionale Galileo and at the 2.5 m Nordic Optical Telescope covering the near-infrared and visible range, respectively. The range from 0.5 to 2.5 m, encompassing the 1 and 2 m pyroxene features, allows a mineralogical characterization of these asteroids.en_US
dc.description.abstract[Methods] A preliminary analysis using the classical methods has been applied to establish some constraints on the surface mineralogy of these objects. Then, the Modified Gaussian Method was applied to gain further insight on the possible mineral components present in the surface of the objects.en_US
dc.description.abstract[Results] The comparison between these basaltic asteroids in near Earth orbits and the achondrite basaltic meteorites shows a quite clear mineralogical link, corroborating the long-standing hypothesis of the Near-Earth Objects population as the immediate source of these meteorites.en_US
dc.format.extent918459 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.publisherEDP Sciencesen_US
dc.relation.isversionofPublisher's version-
dc.rightsopenAccessen_US
dc.subjectMinor planetsen_US
dc.subjectAsteroidsen_US
dc.titleBasaltic asteroids in the Near-Earth Objects population: a mineralogical analysisen_US
dc.typeartículoen_US
dc.identifier.doi10.1051/0004-6361:20054347-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361:20054347en_US
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