Ecology of Vibrios in the Oliveri-Tindari Lagoon (Messina), Two-Year Study     

Renata  Zaccone  Ermanno  Crisafi Lucrezia  Genovese 《Marine Ecology》1992,13(2):149-161

Abstract. A two-year ecological study in the Oliveri-Tindari (Messina) brackish water ponds evaluated the quantitative and qualitative distribution of Vibrio species in relation to the physicochemical conditions of the ponds.
The evaluation of 204 samples shows a general relationship between the halophilic vibrios and water temperature. In particular this relationship is stronger for the Vibrio fraction able to grow at 37°C, i. e. , those species related to human infections. On the other hand, the halophilic vibrios show no relation with the index of fecal contamination.
The ecology of V. parahaemolyticus is discussed in relation to the salinity of Marinello pond.
The distribution of V. cholerae non O1, isolated from all ponds, shows that this microorganism can be considered as autochthonous in coastal environments.  相似文献   

The distant activity of short-period comets – I     

E. Mazzotta Epifani  P. Palumbo  M. T. Capria  G. Cremonese  M. Fulle  L. Colangeli 《Monthly notices of the Royal Astronomical Society》2007,381(2):713-722

  相似文献   

High-resolution observations of the near-infrared emission from NGC 6822 Hubble V     

Sungho Lee  Soojong Pak  Sang-Gak Lee  Christopher J. Davis  Michael J. Kaufman  Kenji Mochizuki  Daniel T. Jaffe 《Monthly notices of the Royal Astronomical Society》2005,361(4):1273-1280

  相似文献   

●●以下19篇文章网络预出版（在线出版）于2023年8月20日，预计刊于《地质论评》2023年第69卷第5、6期或2024年第70卷第1期(2023年9、11月或2024年1月15日发行纸质版）     

毕岭  肖玲  贾慧  章宏波  陈曦 《地质论评》2023,69(4):2023040010-2023040011

遗迹化石是研究古环境、古气候、地层旋回性及其全球成因动力学研究的有效载体。遗迹化石是某种环境条件下生物行为习性的直接证据,是沉积环境的灵敏指示剂,对探讨生物行为习性的演化、生物的多样性、生物地层学、事件地层学、储层地质学等都具有重要的理论意义和应用价值。基于此,本文选取CNKI核心合集数据库中的数据,对1954~2022年遗迹化石相关文献进行系统整理,采用Microsoft Excel 2016和CiteSpace 6.1.R2 软件对文献类型分布、年度发文数量、国家、机构、期刊、作者、高引文献、突现关键词等进行分析,构建和绘制各单元间相互关系,以探求研究领域关键路径及知识拐点,进而挖掘所蕴含的新知识,预测学科研究趋势。研究表明：①我国遗迹化石领域研究发文量最多的机构是河南理工大学;发文量最多的学者是胡斌;被引频次最多的论文作者是龚一鸣;我国遗迹化石的研究主要以国家层面的基金资助为主。②系统发展阶段,我国遗迹化石研究区主要集中在贵阳、新疆;创新发展阶段,研究区主要集中在河南、四川等地。③中国寒武系的遗迹化石研究主要集中在河南省、云南省和贵州省境内;奥陶系、志留系和泥盆系中的遗迹化石研究主要集中在贵州、陕西、新疆塔里木盆地、准噶尔盆地、湖南等地。石炭系—二叠系的遗迹化石研究主要集中在新疆准噶尔盆地西北部、柴达木盆地南缘等地;三叠系的遗迹化石研究主要集中在扬子地区。本文基于新的研究思路和方法,系统分析了国内遗迹化石研究现状和趋势,对于进一步了解遗迹化石具有指导意义。  相似文献   

基于文献计量学的制氢与CCUS技术耦合研究现状及趋势分析     

曹小敏  李琦  徐亮 《高校地质学报》2023,29(1):110-119

氢能是未来能源的“终极形态”,目前工业上主要的制氢方式为化石燃料制氢。CO₂捕集、利用和封存(CCUS)技术是实现氢气从“灰氢”向“蓝氢”转变的重要手段,对国家“双碳目标”的实现至关重要。文章以Web of Science核心合集数据库为数据源,利用CiteSpace软件对制氢与CCUS技术耦合领域的文献来源、研究力量、研究热点和研究前沿进行分析。结果表明,中国的发文量居于世界首位,与其他国家有着广泛的合作基础,国内外研究所和高校为主要研究力量;吸附强化甲烷蒸汽重整(SESMR)制氢技术、化学链燃烧(CLC)制氢技术以及催化剂、吸附剂、载氧体为主要的研究热点;金属载氧体处在研究前沿,研发具有催化和吸附作用的复合催化剂与应用CLC技术和煤气化结合的电、氢联产工艺到火电行业是未来研究发展的两大方向;考虑到“双碳目标”的政策压力和碳税的额外支出,配套CCUS的制氢技术仍是一个优选的方案。  相似文献   

A photometric study of a weak-contact binary: V873 Per     

《New Astronomy》2015

We present a photometric study of a weak-contact binary V873 Per. New observations in BVR filter bands showed asymmetric light curves to be a negative type of the O’Connell effect, which can be described by magnetic activity of a cool spot on the more massive component. Our photometric solutions showed that V873 Per is a W-type with a mass ratio of q = 2.504(±0.0029), confirming the results of Samec et al. (2009). The derived contact degree was found to be f = 18.10%(±1.36%). Moreover, our analysis found the cyclic variation with the period of about 4 yr that could be due to existence of the third companion in the system or the mechanism of magnetic activity cycle in the binary. While available data indicated that the long-term orbital period tends to be stable rather than decreasing.  相似文献   

Constraints on black hole accretion in V Puppis     

Thomas J. Maccarone  Robert P. Fender  Christian Knigge  A. K. Tzioumis 《Monthly notices of the Royal Astronomical Society》2009,393(3):1070-1072

In light of the recent suggestion that the nearby eclipsing binary star system V Puppis has a dark companion on a long orbit, we present the results of radio and X-ray observations of it. We find an upper limit on its radio flux of about 300 μJy and a detection of it in the X-rays with a luminosity of about  3 × 10³¹  erg s⁻¹, a value much lower than what had been observed in some of the low angular resolution surveys of the past. These data are in good agreement with the idea that the X-ray emission from V Puppis comes from mass transfer between the two B stars in the system, but can still accommodate the idea that the X-ray emission comes from the black hole accreting stellar wind from one or both of the B stars.  相似文献   

Optical spectroscopy and Doppler tomography of Cygnus X-2     

P. Elebert  P. J. Callanan  M. A. P. Torres  M. R. Garcia 《Monthly notices of the Royal Astronomical Society》2009,395(4):2029-2038

We present phase resolved optical spectroscopy and Doppler tomography of V1341 Cygni, the optical counterpart to the neutron star low-mass X-ray binary (LMXB) Cygnus X-2 (Cyg X-2). We derive a radial velocity (RV) curve for the secondary star, finding a projected RV semi-amplitude of   K ₂= 79 ± 3 km s⁻¹  , leading to a mass function of  0.51 ± 0.06 M_⊙, ∼30  per cent lower than the previous estimate. We tentatively attribute the lower value of K ₂ (compared to that obtained by other authors) to variations in the X-ray irradiation of the secondary star at different epochs of observations. The limited phase coverage and/or longer timebase of previous observations may also contribute to the difference in K ₂. Our value for the mass function implies a primary mass of  1.5 ± 0.3 M_⊙  , somewhat lower than previous dynamical estimates, but consistent with the value found by analysis of type-I X-ray bursts from this system. Our Doppler tomography of the broad He  ii λ4686 line reveals that most of the emission from this line is produced on the irradiated face of the donor star, with little emission from the accretion disc. In contrast, the Doppler tomogram of the N  iii λ4640.64 Bowen blend line shows bright emission from near the gas stream/accretion disc impact region, with fainter emission from the gas stream and secondary star. This is the first LMXB for which the Bowen blend is dominated by emission from the gas stream/accretion disc impact region, without comparable emission from the secondary star. This has implications for the interpretation of Bowen blend Doppler tomograms of other LMXBs for which the ephemeris may not be accurately known.  相似文献   

Multicolor photometry and polarimetry of the young binary system V1696 Cyg     

K. A. Antonyuk 《Bulletin of the Crimean Astrophysical Observatory》2009,105(1):56-59

We present results of multicolor photometric and polarimetric observations of the binary system V1696 CYG obtained in the Crimean Astrophysical Observatory in 2006. It is shown that observed variations of the linear polarization of the V1696 Cyg light are well correlated with the orbital period phase. We also found brightness variations (～0.1 ^m ) in the UBVRI bands. The brightness variations are weakly correlated with the orbital period phase. A rapid photometric variability was found.  相似文献   

氢化物发生-原子荧光光谱法测定土壤中水溶态和可交换态锑(Ⅲ)和锑(Ⅴ)   总被引：2，自引：2，他引：0  

于兆水  张勤 《岩矿测试》2010,29(1):34-38

在0.10 mol/L酒石酸介质中,采用氢化物发生-原子荧光光谱法测定土壤中水溶态和可交换态Sb(Ⅲ)和Sb(Ⅴ)。以氢气发生器为氩-氢火焰提供氢气,明显降低了硼氢化钾浓度,改善了测定检出限。考察了酒石酸掩蔽Sb(Ⅴ)的量及共存干扰元素的允许量。方法检出限Sb(Ⅲ)为0.026 ng/L,总Sb为0.019 ng/L。加标回收试验表明,方法准确、可靠。  相似文献