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991.
V. F. Esipov E. A. Kolotilov J. Mikolajewska U. Munari A. A. Tatarnikova A. M. Tatarnikov T. Tomov B. F. Yudin 《Astronomy Letters》2000,26(3):162-176
The photometric UBV observations of AS 338 that we began after its outburst in 1983 are presented. They were accompanied by yearly spectroscopic observations and by occasional estimations of the star’s infrared JHKL magnitudes. In June 1993, the star’s optical spectrum was extended to the ultraviolet via IUE observations of AS 338. Collectively, the above observations make it possible to trace the evolution of stellar activity over a period of 15 years in various spectral ranges. In particular, a short-time return of the hot component of AS 338 to the state when He II lines reappeared in the star’s spectrum was noted in 1993. At this time, a blend of the C IV λλ5802 and 5812 lines, which is typical of Wolf-Rayet spectra, was detected in it. In June 1993, the temperature of the hot component was T h ≈ 8.8 × 104 K, and the ratio of its bolometric flux to that of the red giant was F h, bol/F g, bol ≈ 1.0. In August, its temperature increased to ~1.0×105 K, while the bolometric flux dropped by a factor of ~1.5(F h, bol/F g, bol ≈ 0.7). In the B-V, U diagram, the points referring to this so-called quiescent state form a separate group shifted in B-V from all the remaining ones located in a horizontal strip with $\Delta U \approx 3\mathop .\limits^m 5$ and $\Delta (B - V) \approx 0\mathop .\limits^m 4$ . This allows us to diagnose the state of the hot component without spectroscopic observations of the star. In October 1993, the hot component flared up again. The main brightness rise took no more than 19 days. The outburst occurred shortly before eclipse egress of the hot component, whose duration was ~0.01P orb. In December 1993, F h, bol/F g, bol≤1.5 at maximum light. During the recurrent, even stronger outburst in April 1995, F h, bol/F g, bol≤3.4. The Hαline during outbursts has a P Cyg profile and broad wings stretching to velocities of ±1500 km s?1. The color temperature of the active hot component at short optical wavelengths and in the ultraviolet lies in the range of effective temperatures for hot supergiants. Nevertheless, it always produces an H II region in the circumstellar envelope that is larger in size than this binary system. 相似文献
992.
柱撑蛭石吸附去除废水中重金属离子的实验研究 总被引:2,自引:0,他引:2
分别利用有机柱化剂十二烷基磺酸钠(SDS)和无机柱化剂聚羟基铝(HA)对蛭石进行柱撑制得十二烷基磺酸钠柱撑蛭石(SDS-V erm icu lite)和聚羟基铝柱撑蛭石(HA-V erm icu lite),并通过XRD、红外光谱、ZETA电位等表征手段对柱撑蛭石进行表征,同时针对柱撑蛭石对Cu2 ,Cd2 ,C r3 3种重金属离子的吸附进行研究,结果表明:吸附去除率受反应时间、重金属离子的初始浓度、pH值等因素的影响,经柱撑后的蛭石对重金属离子吸附的吸附性能比蛭石原矿要强。柱撑蛭石吸附3种重金属离子的动力学吸附过程可用E lov icb方程和双常数方程进行较好的拟合。 相似文献
993.
994.
潜江盐湖盆地是我国内陆独一无二的高盐度盐湖沉积盆地。本文在分析其岩性韵律特征的基础上,探讨了潜江盐湖生储盖组合特征。研究表明,潜江凹陷潜江组是在干湿频繁交替的古气候条件下,在高盐度、强蒸发、还原—强还原水体中,由北部单向碎屑物源及凹陷周缘卤水与盐源补给形成的盐系地层,岩性组合的有序变化形成了多套生储盖组合系统,不但反映出潜江盐湖沉积的特殊性和复杂性,而且具有十分优越的成油气地质条件。 相似文献
995.
在阿尔金走滑断裂与祁连山北缘逆冲断裂带交汇的酒西盆地出露年龄约为85Ma的富锆安山岩脉,切割年龄大约为105Ma的基性熔岩(粗面玄武岩和玄武安粗岩)。这条安山岩脉具有十分特殊的地球化学特征,具体表现为 (1)强烈过碱性,Na2O K2O达11.8%,A/CNK比值为0.5540;(2)强烈富集高场强元素(HFSE),如Zr(1421μg/g),Hf (26.4μg/g),Y(48.2μg/g),Nb(104.0μg/g),Ta(8.5μg/g)等;(3)明显的Ce正异常;(4)近平直的MREE和HREE稀土配分模式;(5)与基性熔岩相似的初始Sr但明显较低的Nd同位素比值(大于28εNd单位)。这些差异性不仅反映了它们各自源区地球化学特征的差异性,而且反映了部分熔融和岩浆后期演化过程中主要矿物和副矿物溶解或结晶行为的差异性。分析表明,钙长石的结晶分离作用和部分熔融过程中锆石溶解程度的升高是导致该岩脉异常地球化学特征的主控因素。该岩脉所揭示的地球化学过程有助于解译青藏高原内部中生代以来的相似中酸性碱性火山岩的成因。 相似文献
996.
997.
INTRODUCTION The properties of phosphor usedin a plasma dis-play panel (PDP) affect the performance of the PDP(Okazaki et al .,2000 ; Rao and Devine ,2000) . Theluminescent properties of the phosphor are decided bythe morphology ,particle size and size distribution ofthe powder ,sothe requirements for the powder mor-phology are high in a color PDP which belongs to ahigh resolution display apparatus (I m et al .,2005 ;Yang et al ., 2005) . Studies have shown that withsmall particle si… 相似文献
998.
南海1∶100万永暑礁幅海洋区域地质调查成果 总被引:1,自引:0,他引:1
1∶100万永暑礁幅海洋区域地质调查成果揭示了该区地壳的浅、中、深层地质特征。浅层主要研究海底地形、地貌、表层沉积物、矿产资源、潜在地质灾害等;中层主要研究新生代地层、断裂体系、岩浆岩、含油气盆地远景等;深层则研究磁性基底、深层断裂、莫霍面分布特征等。本成果在以下几方面有重要突破:①通过对比新生代以来的地层,确定各沉积盆地地层特征和相互关系,在此基础上预测油气资源前景;②分析表层沉积物类型,预测本区未来可能具有开发价值的固体矿产资源;③利用磁性基底和莫霍面数据分析本区地壳结构特征。 相似文献
999.
Late Pleistocene–Holocene environments in Valle Carbajal, Tierra del Fuego, Argentina 总被引:1,自引:0,他引:1
Ana María Borromei Andrea Coronato Mirta Quattrocchio Jorge Rabassa Silvia Grill Claudio Roig 《Journal of South American Earth Sciences》2007,23(4):321-335
The authors discuss Late Pleistocene–Holocene depositional environments in one of the Fuegian Andes valleys on the basis of palynological, geomorphological, and sedimentological analyses from two sites located near the Beagle Channel. The results obtained at these localities reinforce and refine the Late Pleistocene–Holocene climatic pattern previously recorded there. A colder period, associated with the Younger Dryas stadial event, is suggested by low Nothofagus pollen frequency, and communities of grass, low scrub, and shrub heath expanded into the low/middle slopes (10,310 14C yr BP). By ca. 9500 14C yr BP, warmer and drier conditions occurred, as evidenced by the development of open-grown vegetation in the valley floors (pollen zone O-3), followed by the expansion of open Nothofagus woodland (pollen zone O-2) in the middle Holocene. The milder climate subsequently changed, as indicated by the spreading of the closed forest and mire (pollen zone O-1), to more humid and cooler conditions during the last ca. 5000 yr BP. 相似文献
1000.
Jean-Franois Pastre Agns Gauthier Sbastien Nomade Paul Orth Ana Andrieu Franck Goupille Herv Guillou Stphane Kunesch Stphane Scaillet Paul Randall Renne 《Comptes Rendus Geoscience》2007,339(16):987-997
The Alleret maar (Massif Central, France) provides a long lacustrine sequence (40.6 m) attributed to the early Middle Pleistocene. Sediment, pollen and diatoms analysis of its upper part (AL2 core, 14.6 m) indicates two temperate phases marked by high lake levels, forest development and vegetation expansion. They are separated by a cold period during which lake level drops, coarse sediment input increases and steppic and xerophilous plants develop. Pollen data suggests that this sequence belongs to the upper part of the Cromerian complex. These results are in agreement with the 557 ± 3 ka (±12 ka, including all errors) 40Ar/39Ar age obtained from an interbedded tephra layer emitted by the Mont-Dore/Sancy strato-volcano and establish that this sequence probably covers the MIS 15 substages. 相似文献