排序方式： 共有47条查询结果，搜索用时 31 毫秒
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G.L. Granato L. Silva A. Bressan C.G. Lacey C.M. Baugh S. Cole C.S. Frenk 《Astrophysics and Space Science》2001,277(1):79-82
Recently (Granato, Lacey, Silva et al., 2000, astro-ph/0001308)we have combined our spectrophotometric galaxy evolution code which includes dust reprocessing (GRASIL, Silva et al., 1998) with semi-analytical galaxy formation models (GALFORM, Cole et al. 1999). One of the most characteristic features of the former is that the dust is divided in two main phases: molecular cloud complexes, where stars are assumed to be born, and the diffuse interstellar medium. As a consequence, stellar populations of different ages have different geometrical relationships with the two phases, which is essential in understanding several observed properties of galaxies, in particular those undergoing major episodes of star formation at any redshift. Indeed, our merged GRASIL+GALFORM model reproduces fairly well the SEDs of normal spirals and starbursts from the far-UV to the sub-mm and their internal extinction properties. In particular in the model the observed starburst attenuation law (Calzetti, 1999) is accounted for as an effect of geometry of stars and dust, and has nothing to do with the optical properties of dust grains. 相似文献
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Laura Silva Gian Luigi Granato Alessandro Bressan Cedric Lacey Carlton M. Baugh Shaun Cole Carlos S. Frenk 《Astrophysics and Space Science》2001,276(2-4):1073-1078
We present the basic features and preliminary results of the interface between our spectrophotometric model GRASIL (which
calculates galactic SEDs from the UV to the submm with a detailed computation of dust extinction and thermal reemission) with
the semi-analytical galaxy formation model GALFORM (which computes galaxy formation and evolution in the hierarchical scenario,
providing the star formation history as an input to our model). With these two models we are able to synthesize simulated
samples of a few thousand galaxies for statistical studies of galaxy properties to investigate galaxy formation and evolution.
There is good agreement with the available SED and luminosity function data.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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The spatial characterization of turbulence around large roughness elements in a gravel-bed river 总被引：2，自引：0，他引：2
This study characterizes the flow field above and around multiple instream submerged cobbles, boulders, and pebble clusters in order to obtain a better understanding of the hydrodynamics associated with large roughness elements (LREs) in gravel-bed rivers. Spatially distributed high frequency, three-dimensional velocity measurements were recorded in situ using acoustic Doppler velocimeters at different flow stages. The spatial distributions of turbulent kinetic energy, ke, longitudinal component integral timescales, ITSu, and Reynolds shear stresses were characterized and are presented for selected sites. The longitudinal–vertical Reynolds shear stress increased with flow stage more strongly than the longitudinal–lateral or lateral–vertical Reynolds shear stresses and dominate at the highest measured flows. Canonical redundancy analysis was used to relate LRE morphometrics and mean flow conditions to the turbulence parameters estimated in the LRE wakes (i.e., ke, ITSu, and Reynolds shear stresses). LRE size and mean unobstructed velocity explained the highest proportion of the variance in the turbulent wake statistics. Multivariate regression models based on LRE width, mean unobstructed longitudinal velocity and flow depth are presented offering a tool to predict LRE wake turbulence. 相似文献
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Mauro N. Tammone Adan Hajduk Pablo Arias Pablo Teta Eileen A. Lacey Ulyses F.J. Pardiñas 《Quaternary Research》2014
Comparisons of historical and modern assemblages of mammals can yield important insights into patterns and processes of environmental change. Here, we present the first analyses of small mammal assemblages present in northern Patagonia during the last glacial maximum (LGM). Using remains obtained from owl pellets excavated from an archeological cave site (Arroyo Corral I, levels VII–V, carbon dates of 22,400–21,530 cal yr BP), we generate estimates of the minimum number of individuals for all species detected; these estimates, in turn are used to determine relative species abundances. Comparisons of these data with similar analyses of small mammal remains obtained from a second archeological site (ACoII, levels IV–V, carbon dates of 10,010–9220 cal yr BP) as well as from modern owl pellets reveal pronounced changes in relative species abundance since the LGM. In particular, Euneomys chinchilloides and Ctenomys sociabilis – the predominant species during the LGM – declined markedly, suggesting a change from open, bare habitat punctuated by patches of wet meadows and shrubs to the more densely vegetated mosaic of ecotone habitats found in this region today. These data provide important new insights into the environmental changes that have occurred in northern Patagonia over the last 20,000 years. 相似文献
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Rowena K. Malbon C. M. Baugh C. S. Frenk C. G. Lacey 《Monthly notices of the Royal Astronomical Society》2007,382(4):1394-1414
We incorporate a model for black hole growth during galaxy mergers into the semi-analytical galaxy formation model based on ΛCDM proposed by Baugh et al. Our black hole model has one free parameter, which we set by matching the observed zero-point of the local correlation between black hole mass and bulge luminosity. We present predictions for the evolution with redshift of the relationships between black hole mass and bulge properties. Our simulations reproduce the evolution of the optical luminosity function of quasars. We study the demographics of the black hole population and address the issue of how black holes acquire their mass. We find that the direct accretion of cold gas during starbursts is an important growth mechanism for lower mass black holes and at high redshift. On the other hand, the re-assembly of pre-existing black hole mass into larger units via merging dominates the growth of more massive black holes at low redshift. This prediction could be tested by future gravitational wave experiments. As redshift decreases, progressively less massive black holes have the highest fractional growth rates, in line with recent claims of 'downsizing' in quasar activity. 相似文献
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