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91.
We present results of an analysis of the properties of spheroid-like galaxies that form in hydrodynamical, self-consistent
cosmological simulations run with the DEVA code. We find that the structural, dynamical and X-ray properties, as well as their
correlations, are compatible with observations of early-type galaxies at low z.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
92.
Helen Rovithis-Livaniou Sotirios Tsantilas Peter Rovithis DrahomÍr Chochol AugustÍn Skopal Theodor Pribulla 《Astrophysics and Space Science》2005,296(1-4):101-104
The orbital period variations of the eclipsing binary BX And are examined analysing its (O–C) diagram 1) with the standard method, in which the minima times are fitted by the quadratic ephemeris combined with an assumed light-time effect, and 2) with the first continuous method. The results from the use of the two methods are, as was expected,
different. 相似文献
93.
We report on preliminary results from an ongoing study of star-forming galaxies in the Virgo Cluster with the aim of understanding
the role played by the environment on their evolution. First, the chemical evolution of nine spiral galaxies located in the
inner parts of the cluster has been studied using chemical abundances recomputed for a sample of HII regions. Second, long-slit
optical spectroscopy has been obtained for 22 blue dwarf galaxies selected across the Virgo central field. This sample is
a subset of a larger list of dwarf galaxies for which deep Hα imaging has been collected. Chemical abundances have been derived
for the sample using either a direct estimation of the electron temperature or empirical calibrations. Abundance results correlate
with blue and near infrared magnitude, total HI mass and color.
This revised version was published online in September 2006 with corrections to the Cover Date. 相似文献
94.
During the Late Tortonian, shallow‐water temperate carbonates were deposited in a small bay on a gentle ramp linked to a small island (Alhama de Granada area, Granada Basin, southern Spain). A submarine canyon (the ‘Alhama Submarine Canyon’) developed close to the shoreline, cross‐cutting the temperate‐carbonate ramp. The Alhama Submarine Canyon had an irregular profile and steep slopes (10° to 30°). It was excavated in two phases reflected by two major erosion surfaces, the lowermost of which was incised at least 50 m into the ramp. Wedge‐shaped and trough‐shaped, concave‐up beds of calcareous (terrigenous) deposits overlie these erosional surfaces and filled the canyon. A combination of processes connected to sea‐level changes is proposed to explain the evolution of the Alhama Submarine Canyon. During sea‐level fall, part of the carbonate ramp became exposed and a river valley was excavated. As sea‐level rose, river flows continued along the submerged, former river‐channel, eroding and deepening the valley and creating a submarine canyon. At this stage, only some of the transported conglomerates were deposited locally. As sea‐level continued to rise, the river mouth became detached from the canyon head; littoral sediments, transported by longshore and storm currents, were now captured inside the canyon, generating erosive flows that contributed to its excavation. Most of the canyon infilling took place later, during sea‐level highstand. Longshore‐transported well‐sorted calcarenites/fine‐grained calcirudites derived from longshore‐drift sandwaves poured into and fed the canyon from the south. Coarse‐grained, bioclastic calcirudites derived from a poorly sorted, bioclastic ‘factory facies’ cascaded into the canyon from the north during storms. 相似文献
95.
JUAN PEDRO RODRÍGUEZ‐LÓPEZ NIEVES MELÉNDEZ POPPE L. DE BOER ANA ROSA SORIA 《Sedimentology》2008,55(5):1253-1292
The existence of a mid‐Cretaceous erg system along the western Tethyan margin (Iberian Basin, Spain) was recently demonstrated based on the occurrence of wind‐blown desert sands in coeval shallow marine deposits. Here, the first direct evidence of this mid‐Cretaceous erg in Europe is presented and the palaeoclimate and palaeoceanographic implications are discussed. The aeolian sand sea extended over an area of 4600 km2. Compound crescentic dunes, linear draa and complex aeolian dunes, sand sheets, wet, dry and evaporitic interdunes, sabkha deposits and coeval extradune lagoonal deposits form the main architectural elements of this desert system that was located in a sub‐tropical arid belt along the western Tethyan margin. Sub‐critically climbing translatent strata, grain flow and grain fall deposits, pin‐stripe lamination, lee side dune wind ripples, soft‐sediment deformations, vertebrate tracks, biogenic traces, tubes and wood fragments are some of the small‐scale structures and components observed in the aeolian dune sandstones. At the boundary between the aeolian sand sea and the marine realm, intertonguing of aeolian deposits and marine facies occurs. Massive sandstone units were laid down by mass flow events that reworked aeolian dune sands during flooding events. The cyclic occurrence of soft sediment deformation is ascribed to intermittent (marine) flooding of aeolian dunes and associated rise in the water table. The aeolian erg system developed in an active extensional tectonic setting that favoured its preservation. Because of the close proximity of the marine realm, the water table was high and contributed to the preservation of the aeolian facies. A sand‐drift surface marks the onset of aeolian dune construction and accumulation, whereby aeolian deposits cover an earlier succession of coastal coal deposits formed in a more humid period. A prominent aeolian super‐surface forms an angular unconformity that divides the aeolian succession into two erg sequences. This super‐surface formed in response to a major tectonic reactivation in the basin, and also marks the change in style of aeolian sedimentation from compound climbing crescentic dunes to aeolian draas. The location of the mid‐Cretaceous palaeoerg fits well to both the global distribution of other known Cretaceous erg systems and with current palaeoclimate data that suggest a global cooling period and a sea‐level lowstand during early mid‐Cretaceous times. The occurrence of a sub‐tropical coastal erg in the mid‐Cretaceous of Spain correlates with the exposure of carbonate platforms on the Arabian platform during much of the Late Aptian to Middle Albian, and is related to this eustatic sea‐level lowstand. 相似文献
96.
97.
C. PONCE J. F. SIMANCAS A. AZOR D. J. MARTÍNEZ POYATOS G. BOOTH‐REA I. EXPÓSITO 《Journal of Metamorphic Geology》2012,30(7):625-638
The early (Devonian) collisional stage in SW Iberia has been investigated through the analysis of deformation in the Cubito‐Moura schists, the main lithology of an Allochthonous Complex putatively rooted in the suture between the Ossa‐Morena and South Portuguese zones. The first deformation in these schists (D1) is recorded as a S1‐L1 mylonitic fabric well preserved in early quartz veins. Subsequent D2 deformation caused the main folds and the main (S2) foliation. After restoration, the stretching lineation (L1) trends at a small angle with the Ossa‐Morena/South Portuguese suture. This trend, together with the top‐to‐the‐east kinematics determined from quartz microfabric is indicative of an oblique left‐lateral collisional scenario in SW Iberia. Chlorite–white K‐mica–quartz ± chloritoid multi‐equilibrium calculations yield P–T conditions in the range 0.9–1.2 GPa and 300–400 °C, during the first collisional stage. P–T conditions during D2 were 0.3–0.8 GPa and 400–450 °C, thus indicating an important stage of exhumation of the Allochthonous Complex during these two collisional events, after subduction of the Ossa‐Morena Zone margin under the South Portuguese Zone continental crust. In the general context of the Variscan orogen, dominated by dextral collision, the left‐lateral convergence in SW Iberia can be explained in terms of the Avalonian salient represented by the South Portuguese Zone, which would impinge between Iberia and Morocco. 相似文献
98.
Biochronological data inferred from the Early Pleistocene small mammals of the Barranc de la Boella site (Tarragona,north‐eastern Spain) 
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JAROMÍR NEbreveMEC 《水文科学杂志》2013,58(2):70-73
Abstract For needs of planning and design, data on rainfall duration-intensity-frequency relations are necessary. For this purpose, a network of recording raingages has to be designed. Czechoslovakia has a relatively very dense network with considerably lengthy records. Analysis of this network and particularly of parameters of a new formula for rain intensity-duration-frequency relation, abstracted from this network observations, show that in conditions of a mountainous terrain, no geographical pattern related to topographical characteristics can be evaluated to limit the density of the network. On the other hand, the use of adequate statistical procedure can reduce the necessary lenght of records for the evaluation of reliable data of low frequency, which permits a rational and economical design of permanent and non-permanent networks. 相似文献
100.
JUAN L GARCÍA 《Geografiska Annaler: Series A, Physical Geography》2012,94(4):459-479
Most of the last glacial maximum (LGM) glacier record west of the southern Andes (40–55° S) is today submerged under the Pacific Ocean and therefore the Archipiélago de Chiloé (42–43° S) provides an unusual opportunity to study local sediment and landform associations to help understand paleoglacial features of the former Patagonian ice sheet (PIS). In this context, this work presents the first comprehensive glacial geomorphologic mapping of the central region of the Archipiélago de Chiloé, which is located in a transitional geomorphic region between the Chilean Lake District (CLD, 39–41° S, 73° W) and northwest Patagonia (～43–48° S, 74° W). The Chilotan glacial geomorphology and sediment associations resulted from a warm‐based glacier that characterizes a typical active glacial temperate landsystem, which in central Chiloé combines deposits and landform units originated in subglacial and subaerial environments. Paleoglacial features that occur in central Chiloé are characteristic of an ice‐sheet style of glaciation, which differentiates it from a typical Alpine glacial style defined previously for the CLD. Therefore, the Archipiélago de Chiloé represents a geographical break point where the PIS became the large ice mass that occupied the Patagonian Andes during the last glacial period (Llanquihue Glaciation). A double ice‐contact slope on the east face of the Cordillera de La Costa provides evidence for the most extensive Early Llanquihue glacial advance on Isla Grande de Chiloé. The most prominent LGM advance in the area occurred at 26 000 cal yr BP, coincident with regional stadial conditions, and is defined by a big moraine along the east coast of the island. 相似文献