皱纹盘鲍脓疱病病原菌──河流弧菌-Ⅱ的抗药机制的初步研究     

李太武  丁明进  宋协民  相建海  刘瑞玉 《海洋与湖沼》1996,27(6):637-645

1993年9月至1995年末，大连地区的一龄鲍至成鲍都出现了脓疱病，用常规方法从3个养殖厂的病鲍中分离到了3个菌株，分别为D株、N株和T株。经鉴定这3个菌株为同一种──河流弧菌-Ⅱ。这3个菌株来自3个不同的海区、不同的单位，并且这3个单位使用的抗生素种类和浓度也木同，所以这3个菌株对18种抗生素的敏感度也木同。D株对环丙沙星（抑菌坏直径30mm）、复方新诺明（抑菌坏直径27mm）等敏感，而对青霉素、青霉素Ⅱ、氨苄青霉素（抑菌环直径0mm）等耐药。N株除对青霉素Ⅱ、白霉素、吡哌酸等耐药外，对其它12种抗生素都敏感或中度敏感（抑菌环直径13．5－30mm）。T株对氟派酸（抑菌环直径22mm）、环丙沙星（抑菌环直径20．3mm）等敏感，而对氯霉素、复方新诺明等耐药。研究发现，经常使用同一种抗生素很容易使病原菌产生耐药性．连续3d使用单一的抗生素（青霉素）就会产生耐药的菌株。为证明上述3个菌株的抗药性是属于哪一类，以T株为例，提取总DNA，并对总DNA进行EcoRⅠ酶切图谱分析，图谱有明显的异同，说明3个菌株的抗药性不同可能与基因突变有关。不管是非遗传型还是遗传型，都是由于抗生素为细菌提供了耐药突变株的选择环境，从而使耐药菌株得以大量繁殖。  相似文献   

Tectonic effects of a subducting aseismic ridge: The subduction of the Nazca Ridge at the Peru Trench   总被引：1，自引：0，他引：1  

R. A. Hagen  R. Moberly 《Marine Geophysical Researches》1994,16(2):145-161

A 1987 survey of the offshore Peru forearc using the SeaMARC II seafloor mapping system reveals that subduction of the Nazca Ridge has resulted in uplift of the lowermost forearc by as much as 1500 m. This uplift is seen in the varied depths of two forearc terraces opposite the subducting ridge. Uplift of the forearc has caused fracturing, minor surficial slumping, and increased erosion through small canyons and gullies. Oblique trending linear features on the forearc may be faults with a strike-slip component of motion caused by the oblique subduction of the Nazca Ridge. The trench in the zone of ridge subduction is nearly linear, with no re-entrant in the forearc due to subduction of the Nazca Ridge. Compressional deformation of the forearc due to subduction of the ridge is relatively minor, suggesting that the gently sloping Nazca Ridge is able to slide beneath the forearc without significantly deforming it. The structure of the forearc is similar to that revealed by other SeaMARC II surveys to the north, consisting of: 1) a narrow zone (10 to 15 km across) of accreted material making up the lower forearc; 2) a chaotic middle forearc; 3) outcropping consolidated material and draping sediment on the upper forearc; and 4) the smooth, sedimented forearc shelf.The subducting Nazca plate and the Nazca Ridge are fractured by subduction-induced faults with offsets of up to 500 m. Normal faulting is dominant and begins about 50 km from the trench axis, increasing in frequency and offset toward the trench. These faults are predominantly trench-parallel. Reverse faults become more common in the deepest portion of the trench and often form at slight angles to the trench axis.Intrusive and extrusive volcanic areas on the Nazca plate appear to have formed well after the seafloor was created at the ridge crest. Many of the areas show evidence of current scour and are cut by faulting, however, indicating that they formed before the seafloor entered the zone of subduction-induced faulting.  相似文献   

Intermediate-mass black holes in dwarf galaxies: the case of Holmberg II     

M. Mapelli 《Monthly notices of the Royal Astronomical Society》2007,376(3):1317-1326

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Ultra-Compact H II Regions     

M. G. Hoare 《Astrophysics and Space Science》2005,295(1-2):203-215

This article reviews how observations of dense molecular gas can help us understand the dynamics and evolution of ultra-compact H II (UCHII) regions. Particular attention is paid to the cometary objects, which it is argued are likely to be the dominant class. Thermal molecular lines in emission and absorption are considered as well as the mainly dynamical information from masers. Most of the UCHII regions studied at high resolution have hot cores ahead them which makes interpretation of molecular observations much more complex. Significant support for the champagne flow model for cometary regions can been seen, adding to the evidence from studies of the ionised gas. How the prevalence of cometary objects may fit into a triggered, sequential picture of massive star formation is outlined.  相似文献   

东沙海区海丘发现多底栖方式深水珊瑚     

阎贫  王彦林  靳永斌  赵美霞  钟广见 《地学前缘》2022,29(4):202-210

东沙岛周围海区发育众多深水(200~2 000 m)海丘,其中一些显示了明显的泥火山活动特征。近年的取样调查在多个底质差异明显的海丘都发现了非常丰富的深水珊瑚。为什么这些海丘上深水珊瑚兴盛尚不清楚。根据样品形态分析,初步识别的珊瑚既有以基座紧密固着于碳酸盐岩结核硬底的Madrepora oculate(多眼筛孔珊瑚)、Lochmaeotrochus(灌丛珊瑚)、Enallopsammia(突出海沙珊瑚)、Solenosmilia variabilis、Dendrophyllia(树珊瑚)、 Bamboo Coral (竹节珊瑚)、Golden Gorgonians (金柳珊瑚),还新发现有以鸭蹼状凹凸不平形底壳贴附于海底砂泥级生物碎屑的Desmophyllum dianthus(葵珊瑚)和尖底浅植于碎屑沉积中的Flabellum(扇珊瑚)、Crispatotrochus(卷轮珊瑚)、Balanophyllia(栎珊瑚),还有饼形、杯形能在软质海底缓慢自由移动的Fungiacyathus(蕈杯珊瑚)、Deltocyathusi(角杯珊瑚),指示在底质硬度及海流强度迥异的东沙海丘环境中有多种属珊瑚生长。大量具有机动性的深水珊瑚栖居于弱水动力海底,应更多依赖于栖居地本地而非海流带来的丰富食物,意味着东沙海区的泥火山活动泄漏的烃类流体可能是深水珊瑚食物的主要来源。泥火山的流体活动与珊瑚的兴盛可能具有相互指示意义。  相似文献   

干旱胁迫对莫莫格湿地芦苇叶片光合生理生态的影响机理研究   总被引：3，自引：0，他引：3  

邓春暖  章光新  潘响亮 《湿地科学》2012,10(2):136-141

为了揭示干旱胁迫对芦苇(Phragmites australis)叶片光合生理生态的影响机理,利用LI-6400便携式光合仪和快速叶绿素荧光仪,对干旱胁迫条件下的芦苇叶片光合生理以及芦苇生长状态进行测量分析。结果表明,干旱5d后,芦苇叶片光合速率小幅下降,干旱15d后,其光合速率明显下降,芦苇生长受到显著抑制;干旱胁迫下,芦苇叶片叶绿素含量先增加后减少;芦苇叶片光系统II(PSII)对干旱胁迫反应较敏感,在干旱20d后,其光合电子传递能力和光合性能指数下降,热耗散增加。在干旱胁迫初期,芦苇叶片光合速率的下降以气孔限制为主;在干旱胁迫后期,非气孔限制与气孔限制都起作用,其中非气孔因素主要是指光系统II活性的下降,活性反应中心减少,电子传递能力下降,降低了光系统II的整体光化学性能,进而降低了芦苇叶片的光合速率,抑制了芦苇的生长。  相似文献   

Dynamic evolution model of isothermal voids and shocks     

Yu-Qing Lou  Xiang Zhai 《Astrophysics and Space Science》2009,323(1):17-40

We explore self-similar hydrodynamic evolution of central voids embedded in an isothermal gas of spherical symmetry under the self-gravity. More specifically, we study voids expanding at constant radial speeds in an isothermal gas and construct all types of possible void solutions without or with shocks in surrounding envelopes. We examine properties of void boundaries and outer envelopes. Voids without shocks are all bounded by overdense shells and either inflows or outflows in the outer envelope may occur. These solutions, referred to as type void solutions, are further divided into subtypes and according to their characteristic behaviours across the sonic critical line (SCL). Void solutions with shocks in envelopes are referred to as type voids and can have both dense and quasi-smooth edges. Asymptotically, outflows, breezes, inflows, accretions and static outer envelopes may all surround such type voids. Both cases of constant and varying temperatures across isothermal shock fronts are analyzed; they are referred to as types and void shock solutions. We apply the ‘phase net matching procedure’ to construct various self-similar void solutions. We also present analysis on void generation mechanisms and describe several astrophysical applications. By including self-gravity, gas pressure and shocks, our isothermal self-similar void (ISSV) model is adaptable to various astrophysical systems such as planetary nebulae, hot bubbles and superbubbles in the interstellar medium as well as supernova remnants.   相似文献   

Light element abundances in carbon-enhanced metal-poor stars     

Richard J. Stancliffe 《Monthly notices of the Royal Astronomical Society》2009,394(2):1051-1060

We model the evolution of the abundances of light elements in carbon-enhanced metal-poor (CEMP) stars, under the assumption that such stars are formed by mass transfer in a binary system. We have modelled the accretion of material ejected by an asymptotic giant branch star on to the surface of a companion star. We then examine three different scenarios: one in which the material is mixed only by convective processes, one in which thermohaline mixing is present and a third in which both thermohaline mixing and gravitational settling are taken in to account. The results of these runs are compared to light element abundance measurements in CEMP stars (primarily CEMP- s stars, which are rich in s -processes elements and likely to have formed by mass transfer from an AGB star), focusing on the elements Li, F, Na and Mg. None of the elements is able to provide a conclusive picture of the extent of mixing of accreted material. We confirm that lithium can only be preserved if little mixing takes place. The bulk of the sodium observations suggest that accreted material is effectively mixed but there are also several highly Na and Mg-rich objects that can only be explained if the accreted material is unmixed. We suggest that the available sodium data may hint that extra mixing is taking place on the giant branch, though we caution that the data are sparse.  相似文献   

Metallicities and ages of stellar populations at a high Galactic latitude field     

Michael H. Siegel  Yüksel Karata&#;  I. Neill Reid 《Monthly notices of the Royal Astronomical Society》2009,395(3):1569-1578

We present an analysis of UBVRI data from the selected area SA 141. By applying recalibrated methods of measuring ultraviolet excess (UVX), we approximate abundances and absolute magnitudes for 368 stars over 1.3 deg² out to distances over 10 kpc. With the density distribution constrained from our previous photometric parallax investigations and with sufficient accounting for the metallicity bias in the UVX method, we are able to compare the vertical abundance distribution to those measured in previous studies. We find that the abundance distribution has an underlying uniform component consistent with previous spectroscopic results that posit a monometallic thick disc and halo with abundances of  [Fe/H]=−0.8  and −1.4, respectively. However, there are a number of outlying data points that may indicate contamination by more metal-rich halo streams. The absence of vertical abundance gradients in the Galactic stellar populations and the possible presence of interloping halo streams would be consistent with expectations from merger models of Galaxy formation. We find that our UVX method has limited sensitivity in exploring the metallicity distribution of the distant Galactic halo, owing to the poor constraint on the UBV properties of very metal-poor stars. The derivation of metallicities from broad-band UBV photometry remains fundamentally sound for the exploration of the halo but is in need of both improved calibration and superior data.  相似文献   

Geochemistry of waters associated with the old mine workings at Fonte Santa (NE of Portugal)     

M.E.P. Gomes  I.M.H.R. Antunes  P.B. Silva  A.M.R. Neiva  F.A.L. Pacheco 《Journal of Geochemical Exploration》2010

The quartz veins containing scheelite from Fonte Santa mine cut the Lower Ordovician quartzites. A muscovite–biotite granite (G1) and a muscovite granite (G2), both S-type, crop out close to the Fonte Santa mine and are related to the Moncorvo–Bemposta shear zone. The most altered samples of G2 show intense muscovitization and microclinization and contain chlorite, columbite–tantalite, wolframite, W-ixiolite and Fe-oxides. The tin-bearing granites contain 18 ppm (G1) and 73 ppm (G2) Sn. The most altered samples of G2 correspond to a tungsten granite. The quartz veins contain muscovite, chlorite, tourmaline, scheelite, pyrrhotite, pyrite, sphalerite, chalcopyrite, galena, arsenopyrite, iron oxides, Fe sulfates, phosphates of Pb, Fe and Al. The Fonte Santa mine area was exploited for W between 1942 and 1982. At the end of November 2006, a flood event damaged the tailings dam of Fonte Santa mine, releasing contaminated material and increasing contaminant levels in water within the area of influence of the mine. The waters related to the Fonte Santa mine are poorly mineralized, with electrical conductivity of < 965 µS/cm, and of a mixed type or HCO₃⁻ and SO₄²⁻ types. Most pH values (5.0−8.5) indicate that there is no significant acidic drainage in the region, as found in other areas. More acidic values (pH = 3.4) were found in the mine's lagoon. Waters associated with mineralized veins and old mine activities have Fe and Mn concentrations that forbid their use for human consumption and agriculture. Natural Na, Mg and K water contents are associated with the alteration of albite, chlorite and muscovite of country rock, while Ca with the W-bearing quartz veins. Weathering agents are carbonic and sulphuric acids and the latter has a strong influence in areas draining fine-grained mine tailings.  相似文献