8–13 μm dust emission features in Galactic bulge planetary nebulae     

S. Casassus  P.F. Roche  D.K. Aitken  C.H. Smith 《Monthly notices of the Royal Astronomical Society》2001,327(3):744-750

A sample of 25 infrared-bright planetary nebulae (PNe) towards the Galactic bulge is analysed through 8–13 μm spectroscopy. The classification of the warm dust emission features provides a measure of the C/O chemical balance, and represents the first C/O estimates for bulge PNe. Out of 13 PNe with identified dust types, four PNe have emission features associated with C-based grains, while the remaining 9 have O-rich dust signatures. The low fraction of C-rich PNe, ≲ 30 per cent, contrasts with that for local PNe, around ∼ 80 per cent, although it follows the trend for a decreasing frequency of C-rich PNe with galactocentric radius (Paper I). We investigate whether the PNe discussed here are linked to the bulge stellar population (similar to type IV, or halo, PNe) or the inner Galactic disc (a young and super-metal-rich population). Although 60 per cent of the PNe with warm dust are convincing bulge members, none of the C-rich PNe satisfies our criteria, and they are probably linked to the inner Galactic disc. In the framework of single star evolution, the available information on bulge PNe points towards a progenitor population similar in age to that of local PNe (type I PNe are found in similar proportions), but super-metal-rich (to account for the scarcity of C-rich objects). Yet the metallicities of bulge PNe, as inferred from [O/H], fail to reach the required values – except for the C-rich objects. It is likely that the sample discussed here is derived from a mixed disc/bulge progenitor population and dominated by type IV PNe, as suggested by Peimbert. The much higher fraction of O-rich PNe in this sample than in the solar neighbourhood should result in a proportionally greater injection of silicate grains into the inner Galactic medium.  相似文献   

强振幅地震属性分析技术在车排子地区油气检测中的应用   总被引：3，自引：1，他引：3  

王离迟  洪太元  江洪 《新疆地质》2006,24(3):310-313

准噶尔盆地西缘车排子地区是目前中石化的有利探区,P2井的突破,加速了该区油气勘探的步伐.为了提高勘探的经济效益,用地震特殊处理手段对有利目标进行预测就显得非常重要和迫切.本文运用强振幅属性分析技术有效地预测了该区的有利目标区,并经实钻证实.强振幅属性分析技术是目前车排子地区油气检测的有效手段.  相似文献   

The Alpine evolution of the Southern Alps around the Giudicarie faults: A Late Cretaceous to Early Eocene transfer zone     

Alberto Castellarin  Gian Battista Vai  Luigi Cantelli 《Tectonophysics》2006,414(1-4):203

Data supporting relevant Late Cretaceous–Early Eocene sinistral displacement along the Giudicarie fault zone and a minor Neogene dextral displacement along the Periadriatic lineament are discussed. The pre-Adamello structural belt is present only in the internal Lombardy zone, located W of the Adamello massif. This belt is unknown in the Dolomites and surrounding areas located to the E of the Giudicarie lineament. Upper Cretaceous–Early Eocene thick syntectonic Flysch deposits of Lombardy and Giudicarie are well preserved along the southern and eastern border of the pre-Adamello belt (S-vergent Alpine orogen). Towards the E, in the Dolomites and in the Carnic Alps and external Dinarides, only incomplete remnants of Flysch deposits, Aptian–Albian and Turonian–Maastrichtian in age, are present. They can be considered as equivalent to those of Lombardy and Giudicarie formerly in connection to each other along the N-Giudicarie corridor. To the S, the syntectonic Flysch deposits are laterally replaced by the calcareous red pelagites of the Scaglia Rossa and by the carbonate shelf deposits of the Friuli (to the E) and Bagnolo (to the S) carbonate platforms. The different location in the southern structural accretion of the eastern and western opposite blocks (the Dolomites versus the pre-Adamello belt) can be related to the Cretaceous–Eocene convergence. In this frame, the N-Giudicarie fault has been considered as part of a former transfer zone, which produced the sinistral lateral displacement of the Southern Alps front for an amount of some 50 km. During the Late Eocene to Early Oligocene the transfer zone was mostly sealed by the Paleogene Adamello batholith. Oligocene to Neogene compressional evolution inverted the N-Giudicarie fault into a backthrust of the Austroalpine units over the South-Alpine chain.  相似文献   

准噶尔盆地西北缘车排子地区侏罗系物源及古水流分析   总被引：16，自引：8，他引：16  

胡宗全  朱筱敏  彭勇民 《古地理学报》2001,3(3):49-54

通过岩石岩屑组分分析、重矿物组分分析、倾角测井、地层厚度分析等方法，对准噶尔盆地西北缘车排子地区侏罗系进行物源及古水流方向分析。岩屑组分分析指示着大致的物源前进方向，重矿物分析明确了物源泄入的主要通道，倾角测井在单井点处对古流向有相当高的表现精度，但这三种方法均存在数据平面覆盖率较低和分布密度差异大的缺陷，而运用地震层位解释所得的地层等厚度图则可以在较大尺度上的二维平面内推测沉积时期的古地形，进而可以推测古流向，但它仅是一种间接预测方法，存在局部古流向预测精度较低的不足。文中综合各种方法，将直接预测方法的高精度和间接方法的高覆盖能力结合起来，对古流向作出较高精度的预测。在古流向研究的基础上建立了冲积扇－辫状河－河泛平原沉积体系的沉积相模式。该模式认为对于水流能量保持能力差的冲积扇，其古流向应该沿短轴陡坡降方向，即大致为SEE方向，而对于水流能量保持能力较强的辫状河来说，其古流向应该沿长轴缓坡降方向，即为SE甚至SSE方向。该模式的提出对于提高地震相－沉积相的转相精度具有一定的指导意义。  相似文献   

准噶尔盆地西缘车排子地区砂岩型铀矿成矿潜力及找矿方向     

赵磊 《地质与勘探》2021,57(3):507-517

砂岩型铀矿作为一种重要的铀矿类型,以其开采成本低、环境影响小、经济效益好成为当今铀矿勘查主攻方向。准噶尔盆地周缘具有巨厚的沉积地层和巨大的斜坡带,是我国砂岩型铀矿重要的找矿靶区。本次研究针对准噶尔盆地西缘车排子地区,通过γ测井、矿化砂体地球化学和地下水地球化学特征研究,结合区域构造条件、铀源条件、水文地质条件、矿化砂体地质特征和放射性异常等砂岩型铀矿成矿条件和找矿标志,分析车排子地区砂岩型铀矿成矿方式和可能的找矿方向。研究认为,车排子地区具有优越的砂岩型铀矿成矿地质条件,其中油气还原作用是铀成矿的主要方式,新近系沙湾组是铀成矿的主要层位,砂体的高孔隙度和渗透性以及所处良好的氧化还原环境是有利的铀成矿条件。  相似文献   

准噶尔盆地车排子凸起东缘下切谷特征及其形成机制     

秦磊  李小刚  邱子瑶  李志军  徐少华  李仪汶  陈岑  汪佳蓓  文思奇 《现代地质》2021,35(3):832-840

下切谷是层序地层学研究的重要内容之一,同时也是寻找地层、岩性等圈闭的有利地区。综合利用钻测井、三维地震资料以及地震平面属性信息,在车排子凸起至红—车断裂带区域识别出下切谷沉积体系,对下切谷的发育特征以及形成机制进行分析,结果表明:地震振幅绝对值之和属性体显示研究区发育4条近东西流向的下切谷,主要表现为分支型和单一型的平面形态特征。在地震剖面上,几何形态以V形和U形为主,谷内沉积物充填样式有双向上超充填型和侧向加积充填型,同时具有加积、前积和上超等地震反射特征,属于“顺源堆积”与“溯源堆积”的交互沉积。结合准噶尔盆地车排子凸起中生代构造及气候演化特征分析认为,凸起东缘下切谷形成于晚侏罗世。该时期车排子凸起强烈隆升,相对湖平面急剧下降,河流侵蚀下伏地层导致下切谷形成。下切谷内沉积充填阶段发生在白垩纪。该时期车排子凸起剧烈下沉,相对湖平面上升,下切谷持续性的接受沉积充填。  相似文献   

准噶尔盆地车排子凸起沙湾组油藏输导体系研究   总被引：1，自引：0，他引：1       下载免费PDF全文

王坤  任新成  马奎  黄擎宇  石书缘  高建文 《高校地质学报》2016,22(2):350

新近系沙湾组是准噶尔盆地车排子凸重要的油气富集层位。在对沙湾组油藏分布、油性进行分析的基础上,结合前 人研究成果,将沙湾组油气的成藏过程分为两个阶段：古油藏阶段和次生调整阶段,并分别论述各阶段的输导体系及其时 空组合关系。古油藏阶段主要发育白垩系底部不整合面和红车断裂带同生逆断层组成的输导体系,研究区北部的白垩系底 面不整合有效输导厚度大,向西逐渐减薄为0;同生逆断裂是控制红车断裂带发育演化的主干断裂,形成时间早,断距 大。次生调整阶段则发育有沙湾组一段底部砂体、红车断裂带后生正断层、艾卡断裂带、凸起之上新近系张性断裂组成的 输导体系,沙一段砂体在凸起之上分布广泛,沉积连续而稳定,呈“毯状”自南向北逐渐减薄,做为最底部的砂体层,是 该阶段主要的横向输导体系;新近纪末期红车断裂带发育了一期正断裂,断裂活动强度大且规模较大,凸起之上则发育一 期与红车断裂带后生正断层同期形成的新近系正断层,凸起南部四棵树凹陷的艾卡断裂活动期长、断距大、延伸远,这些 断层构成了次生调整阶段的纵向输导体系。利用运移通道指数（MPI） 及颗粒荧光定量分析（QGF） 分别预测了白垩系底 不整合面及沙一段毯状砂体的优势运移区。平面上将运移通道指数在0.3以上的区域作为不整合输导层的优势运移区,将 QGF指数值大于3.8的区域作为沙一段毯状砂体的优势运移区。通过分析多套输导体系在油气成藏的不同阶段的空间组合以 及油气分布与输导体系的关系,明确了输导体系对油气成藏的控制作用,预测609井区具备油气输导的有利条件,可作为 下步勘探目标区。  相似文献   

准噶尔盆地车排子地区侏罗系八道湾组沉积古地貌及岩性分布^*   总被引：1，自引：0，他引：1       下载免费PDF全文

周路  韦红  唐勇  孔玉华  任本兵  吴勇  关旭 《古地理学报》2013,15(3):383-400

利用三维地震资料,对准噶尔盆地车排子地区侏罗系八道湾组各岩性段精细井震标定与构造解释,厘定出各岩性段在车排子地区的尖灭线位置和尖灭线类型,分析古地貌差异程度对尖灭线形成的控制作用。采用地层厚度法和地震层拉平法研究八道湾组各段沉积古地貌特征,分析断裂对古地貌形成的控制作用,结合构造演化剖面分析古地貌演化和被改造后的特征,开展地震属性、储集层地震反演和沉积相分析,重点分析古地貌对沉积和岩性的控制作用,再现了该地区沉积相及储集层段岩性分布特征。车排子地区八道湾组沉积古地貌起伏明显,呈坡—隆—凹组合特征,斜坡的陡缓程度对沉积相的类型和岩性及其沉积物的粗细具有重要控制作用。八道湾组不同沉积时期低隆起的形态和隆起幅度都存在较大的差别,且隆起幅度越高其聚砂特点越明显,沟谷既是输砂通道,也是聚砂的重要场所,现今砂体的分布与沟谷展布方向关系密切。  相似文献   

XMM‐Newton detection of relativistic Fe emission in the X‐ray spectrum of SAX J1711.6–3808     

C. Snchez‐Fernndez  M. Santos‐Lle  J. J. M. In' t Zand  R. Gonzlez‐Riestra  B. Altieri  R. Saxton  A. J. Castro‐Tirado 《Astronomische Nachrichten》2006,327(10):1004-1007

  相似文献   

Stellar sources in the isogal inner galactic bulge field (l=0°,b= − 1°)     

D. K. Ojha  A. Omont  S. Ganesh  G. Simon  M. Schultheis 《Journal of Astrophysics and Astronomy》2000,21(1-2):77-90

ISOGAL is a survey at 7 and 15 μm with ISOCAM of the inner galactic disk and bulge of our Galaxy. The survey covers ∼ 22 deg² in selected areas of the centrall = ±30 degree of the inner Galaxy. In this paper, we report the study of a small ISOGAL field in the inner galactic bulge (l = 0°,b = −1°, area = 0.033deg²). Using the multicolor nearinfrared data (IJK_s) of DENIS (DEep Near Infrared Southern Sky Survey) and mid-infrared ISOGAL data, we discuss the nature of the ISOGAL sources. The various color-color and color-magnitude diagrams are discussed in the paper. While most of the detected sources are red giants (RGB tip stars), a few of them show an excess in J-K_s and K_s-[15] colors with respect to the red giant sequence. Most of them are probably AGB stars with large mass-loss rates.  相似文献