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7 documentos corresponden a la consulta.
Palabras contadas: neogene: 9
Japas, M.S. - Cortés, J.M. - Pasini, M.
Rev. Asoc. Geol. Argent. 2008;63(2):213-222
2008

Descripción: Triassic clastic and volcanic rocks from the Precordillera were deposited in the Cuyana rift basin filling half-graben systems. Contractional/transpressional Andean tectonics leads to the almost complete inversion of some portions of the basin which resulted in present-day isolated, structurally controlled outcrops of these Triassic rocks. In the Southern Precordillera both the degree of Neogene tectonic inversion and structural compexities are variable. At the regional scale, these variations in Andean deformation are related to first order anisotropies like the Cuyana basin borders and previous shear zones of Permian age (San Rafael orogenic phase). This paper focuses on the kinematic analysis done in the Cerro Manantial thrust sheet area (Cordón San Bartolo, central sector of the South Precordillera) where tectonic inversion was not that strong and the influence of oblique strain zones is practically null. Four sets of extensional/ transtensional faults were recognized affecting Triassic sedimentary rocks of the El Cielo Formation (Uspallata Group) at the Quebrada El Salto. Fault displacements are of decimetric to metric scale. Mesoscopic kinematic indicators (en-échèlon tensional gashes, Riedel shear fractures, sigmoidal fractures) were measured. Once Andean deformation was restored, a NNE direction for the Triassic extension was determined. Considering a northern branch of the Cuyana basin trending NNW (Az. 150°) and oblique to the direction of extension (Az. 35-40°), a sinistral strike-slip component could be inferred for this portion of the basin.
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Tipo de documento: info:ar-repo/semantics/artículo

Mescua, J.F. - Ramos, V.A.
Rev. Asoc. Geol. Argent. 2009;65(1):111-122
2009

Descripción: Results of a detailed geologic survey of the Río Borbollón area, located in the Cordillera Principal of the province of Mendoza are presented. The stratigraphic record of the area corresponds to a Jurassic-early Cretaceous sedimentary succession, the products of Neogene igneous activity and Quaternary deposits. The Tres Esquinas and La Manga Formations of Jurassic age were recognized for the first time in the study area. The main structural features of the area are described and interpreted based on the obtained data and previous works. A balanced structural cross section of the Malargüe fold and thrust belt at 34°15'S depicts the structural style and the amount of orogenic shortening in this region of the Andes.
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Tipo de documento: info:ar-repo/semantics/artículo

Llambías, E.J. - Bertotto, G.W. - Risso, C. - Hernando, I.
Rev. Asoc. Geol. Argent. 2010;67(2):278-300
2010

Descripción: The Payenia basaltic province is a typical retroarc association developed along the foothills of the Andes between 33°40 ́S and 38°00'S. It records two main events, an older, mostly Miocene one (26 to 8 Ma) and a younger Pliocene to Holocene one (younger than 5 Ma). It covers an N-S lowland belt named here the central depression. To the North of 36°20'S, the region was described as Los Huarpes depression, a partially deformed sedimentary basin characterized by a 1000 m-thick, undifferentiated Cenozoic sequence. To the south, Upper Cretaceous to Lower Paleogene layers, instead of the undifferentiated Cenozoic deposits, are covered by basalts. The volcanism additionally covers the western side of the San Rafael Block as well as the fold and thrust belt of the Andean foothills. The Payenia province consists of more than 800 monogenetic basaltic cones, and scarce polygenetic volcanos fed by shallow magmatic chambers. Among the latter, the following examples can be mentioned: Miocene Chachahuén volcano (7 to 5 Ma), composed of andesites, rhyodacites and basalts with high-K and amphibole; Pliocene El Nevado volcano, with calc-alkaline, basaltic trachyandesites, trachytes, dacites and rhyolites; and Upper Pleistocene to Holocene Payún Matrú volcano, composed of trachytes, trachyandesites and trachybasalts. The southernmost area of the central depression is covered by the Pleistocene, Auca Mahuida basaltic shield (1.7 to 0.88 Ma), consisting of trachybasalts, basaltic trachyandesites and trachyandesites. This shield is aligned with Tromen and Domuyo volcanos, defining an NW-SE volcanic belt, oblique to the Andes, whose southern tip corresponds to the Cortaderas lineament. Some of the monogenetic cones are of hydromagmatic origin, whereas a few others exhibit small mantle inclusions. The Payenia retroarc province develops to the south of the Pampean flat slab segment, where the heights of the Andes are smaller. This height difference might have been caused by a higher thermal gradient that softened the crust in the steeper subduction segment, while the colder lithosphere in the flat slab segment allowed greater crustal thickening and height. From the tectonic point of view the height difference has been attributed to a smaller orogenic contraction in the southern segment. Holocene volcanism appears exclusively at Payun Matru volcano. The associated thermal anomaly may explain the segmentation of the central depression, separating the Cenozoic Los Huarpes basin in the north and the section without coeval sedimentation in the south. The only surface evidence of this segmentation is the E-W, La Carbonilla fault, running both sides of the Payun Matru volcano. Other authors have explained this thermal anomaly as a process of crustal thinning and stretching associated with hot injection from the asthenosphere.
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Tipo de documento: info:ar-repo/semantics/artículo

Sellés-Martínez, J. - Azcurra, D.
Rev. Asoc. Geol. Argent. 2010;66(1-2):80-93
2010

Descripción: Structures cropping out in the Jachal Valley from the Cuesta del Viento dam to the locality of Los Tuneles are described and analyzed. These structures affect the Ordovician Yerba Loca and Los Sombreros Formations and the Paleogene-Neogene Vallecito and Rodeo Formations. The oldest units form the heights, Sierra Negra de Rodeo and Sierra de los Túneles, which are limited in their eastern flanks by the La Tranca and Los Blanquitos overthrusts, and by the angular unconformity underlying Rodeo Formation in their western ones. The regional folds show asymmetrical shapes and a wavelength comparable to the width of the Sierras, but minor structures ranging from meters to tens of meters are very common in their eastern limbs. Regional folds axis trend varies from Az 315 to Az 360 and the vergence of pre-carboniferous and andean structures point to the east, what makes very difficult to use orientation as a criterion to discriminate the differentiated deformational episodes. The comparison of sedimentological and structural features in the Rodeo area with those at the San Juan River evidences strong similarities but also important differences. Among the first ones, it can be mentioned the lithological and structural resemblance of the Ordovician units, which show NS trending axis in the eastern outcrops and point N-NW in the western ones. Main differences are the absence -in the Rodeo area- of the metapelites of the Silurian Calingasta Formation. and that of the conglomerates and rhythmites of the Devonian (?) El Planchón Formation. present in the San Juan River section.
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Tipo de documento: info:ar-repo/semantics/artículo

Japas, M.S. - Urbina, N.E. - Sruoga, P.
Rev. Asoc. Geol. Argent. 2010;67(4):494-506
2010

Descripción: Located at the transitional southern end (33o S) of the Pampean flat-slab, the Tertiary volcanic belt records the eastward migration of the Andean volcanic arc due to the flattening of the Nazca Plate in Mio-Pliocene times. The tertiary volcanic belt encompasses several very important metallogenetic districts in the San Luis Pampean Ranges. Volcanic rocks and associated ore-deposits crop out following a NW-WNW trending belt at La Carolina, Cañada Honda - Cerros Largos, Cerros del Rosario and El Morro volcanic fields. The available geochronological data indicate that the volcanic activity began early at the western end of the belt and ended ~ 10 Ma later at its eastern border. Cañada Honda district represents the oldest and longest-lived volcanic field of the tertiary volcanic belt. It records eruptive events and related hydrothermal alteration from 12-13 Ma to 7.3 Ma, including lavas and volcaniclastic products. Preliminary structural analysis shows that previous structures have strongly controlled, either directly or indirectly, the emplacement of volcanic rocks and related mineral deposits. Kinematic and strain fabric analyses allow to recognize two volcano-tectonic associations. One of these associations would be related to dextral reactivations of structures parallel to basement foliation. On the other hand, the main one would be linked with the generation of two volcano-tectonic depressions which are aligned in a NW-WNW direction. Their dominant structures trend NW-WNW and reveal sinistral-normal motions, both at local and Tertiary volcanic belt scales.
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Tipo de documento: info:ar-repo/semantics/artículo

Del Río, C.J.
Nautilus 1997;110(3):77-93
1997

Descripción: Retrotapes, new genus, comprises a group of Neoaustral bivalves that appeared in the southern circumpolar regions by the Eocene and have since been confined to the high latitudes of the southern hemisphere. Its presence in the Tertiary strata of Antarctica and southern South America reflects an active faunal interchange between both regions during the Eocene. Retrotapes is here proposed to include to those Recent and Tertiary representatives of the Subfamily Tapetinae (Family Veneridae) from southern South America and Antarctica that had been previously placed in Venus Linné, 1758, Marcia H. and A. Adams, 1857, Eurhomalea Cossmann,1920, Samarangia Dall,1902, and Kalelysia Römer, 1857. The Argentine Tertiary species Retrotapes ninfasiensis, new species, R. fuegoensis, new species, R. striatolamellata (Ihering, 1897) and R. scutata (Ihering, 1907) are here described and illustrated. The Recent Argentine Venus exalbida Chemnitz, 1795 and Venus lenticularis Sowerby, 1835, the Antarctic V. antarctica Sharman and Newton, 1894 and V. newtoni Wilckens, 1911 (Eocene-early Oligocène?, La Meseta Formation), and the Neogene Chilean species V. navidadis Philippi, 1887 and V. colchaguensis Philippi, 1887 are also included in this new genus.
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Tipo de documento: info:ar-repo/semantics/artículo

Tofalo, O.R. - Etchichury, M.C. - Fresina, M.
Rev. Asoc. Geol. Argent. 2005;60(2):316-326
2005

Descripción: Samples obtained from four wells located at Bancalari, Buenos Aires Province, have been analysed in order to define textural parameters, petrofacies, palaeoenvironments and palaeoclimate evolution. The samples were obtained from the upper part of the Puelches Formation and from the Pampean and Postpampean sediments; in particular this paper highlights the informally named Preensenadense interval. Six textural groups (I to VI) and two petrofacies (A and B) have been recognised. Groups I to III represent fluvial sands (I), gradually overlain by backswamp and lake deposits (II -III), generated on very low slope and well-drained floodplains, with oxidizing conditions. Groups II and III are assigned to Preensenadense interval. The three groups are included in petrofacies A (Qt:F:L = 43:49:8), of sedimentary and basement provenance, which has an igneous metamorphic heavy suite, scarce hornblende and dominance of smectite over illite. By contrast the upper groups (IV to VI) show more varied depositional settings, including aeolian, fluvial and marine environments. Group IV is loessic and corresponds to the Ensenada Formation. Group V, the Lujan Formation (Río Salado Member), is composed of fluvial plain deposits deposited during a wet and temperate climate. Marine silts and clays (group VI) represent a transgression over terrestrial environments and record of the so-called Querandino event. The three upper groups are included in petrofacies B (12:56:32), and have a magmatic arc provenance, with plagioclase dominance and contributions of volcaniclastic and vitroclastic material. It contains a heavy-mineral suite mainly composed of hornblende and it has more illite than smectite. © 2005 Asociación Geológica Argentina.
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Tipo de documento: info:ar-repo/semantics/artículo