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71.
K.S.V.S. Narasimhan P.M.S. Namboodiri S.M. Alladin 《Astrophysics and Space Science》2003,286(3-4):381-395
A series of N-body simulations have been performed to interpret the interacting pair of galaxies VV 117 (NGC 2444/45). The
galaxies have been modelled assuming a mass ratio two. The simulations use various values for the distance of closest approach
and the eccentricity of the relative orbit of the pair. A plausible scenario for the tidal disruption of the less massive
galaxy is proposed. NGC2444, having double the mass of NGC 2445, has undergone penetrating collision with the latter in a
hyperbolic or a parabolic orbit. After the first collision, the orbit has become bound. Our results show that VV 117 has either
just emerged from the first collision or are on the verge of a second collision. NGC 2445suffers considerable disruption and
mass loss. NGC 2444 is not affected much. The second collision is expected to culminate in the merger of the two galaxies.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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73.
Cai-Na Hao Xiao-Yang Xia Shu-De Mao Zu-Gan Deng Hong Wu 《天体物理学报》2008,8(1):12-24
We study the growth of black holes and stellar population in spheroids at high redshift using several (sub)mm-loud QSO samples. Applying the same criteria established in an earlier work, we find that, similar to IR QSOs at low redshift, the far-infrared emission of these (sub)mm-loud QSOs mainly originates from dust heated by starbursts. By combining low-z IR QSOs and high-z (sub)mm-loud QSOs, we find a trend that the star formation rate (M*) increases with the accretion rate (Mace). We compare the values of M*/Macc for submm emitting galaxies (SMGs), far-infrared ultraluminous/hypeduminous QSOs and typical QSOs, and construct a likely evolution scenario for these objects. The (sub)mm-loud QSO transition phase has both high Macc and M* and hence is important for establishing the correlation between the masses of black holes and spheroids. 相似文献
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75.
G. Urbano A.M. Meléndez V.E. Reyes M.A. Veloz I. González 《International Journal of Mineral Processing》2007
The galvanic effect between the main associated mineralogical phases in a mineral sphalerite concentrate was evaluated using an alternative methodology. Comparative voltammetric studies were performed between high purity galena mineral (94.65%) and sphalerite concentrate (content of 78.11% sphalerite, ZnS; 13.64% galena, PbS; 0.57% chalcopyrite, CuFeS2; 0.41% cadmium sulfide, CdS; and 0.11% arsenopyrite, FeAsS) using carbon paste electrodes (CPE) in order to identify galvanic interactions that affect their reactivity. The electrolyte was an aqueous solution of 0.1 M NaNO3 (pH 6.5). The results showed that, in sphalerite concentrate, the electrochemical reactivity of the galena was diminished and displaced to more positive potentials with respect to the high purity galena mineral response. This behavior can be attributed to the galvanic protection offered by the sphalerite on the galena, thereby avoiding its free oxidation. On the other hand, sphalerite oxidation was diminished by the formation of a passive products film that is dissolved to more positive potentials which provokes oxidation of other minerals like CuFeS2, (Zn,Cd)S and FeAsS present in a minor proportion in the sphalerite concentrate. 相似文献
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78.
A study of an expanding seagrass bed on the south-west coast of British Columbia, Canada involved documentation and explanation of the pattern of expansion of the vegetation as well as documentation and experimental investigation of the accompanying changes in the distribution of infaunal invertebrates. Expansion followed a major environmental change, improved water clarity initiated in 1969 when a causeway blocked access to the site for silty Fraser River water. The original eelgrass (Zostera marina) bed expanded landward over 30 m year−1, probably causing more and more water to be retained in the bed at low tide and thus improving its own habitat. More rapid expansion occurred from 1979–1983 after Z.japonica colonized at the landward edge of the eelgrass bed and in a separate intertidal area. Expansion ceased around 1983 coincident with, but probably independent of, further construction.Burrowing shrimp (Callianassa californiensis) decreased in abundance between 1977 and 1984 in areas where the two seagrasses colonized. Short-term experiment over one summer and fall showed that removal of all shoots allowed adult shrimp and tube worms to colonize the sediment while addition of shoots of Z. japonica by transplanting caused temporary decreases in shrimp abundance. After a few weeks an established shrimp population destroyed the transplants. Among reasonable alternate hypotheses for the decline in Callianassa, the effect of sediment texture can be eliminated, but either direct negative effects of seagrass, i.e. inhibition of the burrowing of adult shrimp or of settlement of juveniles, or indirect effects, i.e. the harboring of more predators of shrimp in seagrass beds, deserve further study. 相似文献
79.
Starting out with two interacting Rossby-Haurwitz waves, the generation of zonal flow is discussed. It is shown that zonal flow cannot be generated by first or second order interactions between two such waves, unless they are exchanging energy with a third wave within a resonant triad. The generation of zonal flow at second order through resonant triad interactions is subsequently established and studied. 相似文献
80.
为了揭示高温暖水在中国南海(文中简称南海)夏季风爆发中所起的作用,依据欧洲中期天气预报中心发布的第5代全球大气海洋再分析资料,发现气候平均意义下印度洋—太平洋暖池中30℃以上高温暖水会在5月出现移位:5月上旬高温暖水出现在孟加拉湾中部,而到下旬消退并移位到南海南部。通过分析局地天气尺度的海洋-大气相互作用过程,揭示了上述高温暖水月内移位的物理机制:在孟加拉湾夏季风爆发后,逐渐增强的潜热释放和减少的短波辐射会导致孟加拉湾高温暖水的面积逐渐缩小;与此同时,在副热带高压影响下,南海菲律宾岛西南高温暖水出现,并因其面积逐渐增大,并与泰国湾的高温暖水共同构成了南海南部的高温暖水。研究发现南海季风爆发几乎都出现在上述高温暖水移位之后,因此孟加拉湾中部和南海南部海表温度的差由正转负可以作为南海季风爆发的先兆。
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