A deep X-ray observation of M82 with XMM–Newton     

P. Ranalli †‡  A. Comastri  L. Origlia  R. Maiolino § 《Monthly notices of the Royal Astronomical Society》2008,386(3):1464-1480

We report on the analysis of a deep (100-ks) observation of the starburst galaxy M82 with the EPIC and RGS instruments onboard the X-ray telescope XMM–Newton . The broad-band (0.5–10 keV) emission is due to at least three spectral components: (i) continuum emission from point sources; (ii) thermal plasma emission from hot gas; and (iii) charge-exchange emission from neutral metals (Mg and Si). The plasma emission has a double-peaked differential emission measure, with the peaks at ∼0.5 and ∼7 keV. Spatially resolved spectroscopy has shown that the chemical absolute abundances are not uniformly distributed in the outflow, but are larger in the outskirts and smaller close to the galaxy centre. The abundance ratios also show spatial variations. The X-ray-derived oxygen abundance is lower than that measured in the atmospheres of red supergiant stars, leading to the hypothesis that a significant fraction of oxygen ions have already cooled off and no longer emit at energies ≳0.5 keV.  相似文献   

Spitzer observations of M33 and the hot star, H ii region connection     

Robert H. Rubin  Janet P. Simpson  Sean W. J. Colgan  Reginald J. Dufour  Gregory Brunner  Ian A. McNabb  Adalbert W. A. Pauldrach  Edwin F. Erickson  Michael R. Haas  Robert I. Citron 《Monthly notices of the Royal Astronomical Society》2008,387(1):45-62

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深度学习预测GPS时间序列在探索门源M_S6.4地震前兆中的应用     

陈善鹏  尹玲  梁诗明  胡向阳  余小燕 《大地测量与地球动力学》2020,40(12):1248-1253

以2016-01-21门源M_S6.4地震为例,提出用深度学习预测的GPS时间序列研究地震前兆。用震中附近门源台（QHME）、民乐台（GSML）及古浪台（GSGL）无震时的GPS时间序列训练LSTM神经网络,得到高精度的GPS时间序列预测模型,再分别对该地区无震时和地震前一段时间的GPS时间序列进行回溯性预测。对比预测时间序列与真实时间序列发现,震前2条时间序列大部分的相似性指标比无震时低,说明震前预测时间序列与真实时间序列差异明显,同时考虑震前时间序列的趋势异常,认为出现了异常时段;3个台站分别在E、N、U方向出现多个异常日期,且不同台站具有相同的异常日期,说明探索到了地震前兆。  相似文献   

流动商贩的空间分布特征及与正规商业的分布关系——基于距离测度方法的数量研究   总被引：4，自引：1，他引：3  

张延吉  张磊  吴凌燕 《地理学报》2017,72(4):618-632

有关非正规经济的空间分布特征始终缺乏宏观维度的定量研究。本文利用数字化城市管理系统中的流动商贩数据和工商局登记的正规商业数据,通过DO指数和M函数,分别探究流动商贩的空间特征及其与正规商业的分布关系。研究发现：① 绝大多数类型的流动商贩及其占地面积具有显著集聚的空间格局;其中,与居民需求较为密切的商贩类型,集聚程度相对较低。② 相较于正规商业,流动商贩在极小的空间尺度上更为强烈地集聚分布;但随着尺度扩大,集聚程度呈快速衰减态势。③ 经营内容相近的流动商贩与正规商业之间表现出显著的互斥关系,而非共栖关系;且两者的互斥程度在较小的空间尺度上尤为强烈。由此,本研究证明设立摊贩疏导区具有可行性和必要性,并就设置的类型及原则提出了初步建议。  相似文献   

Excursion to Mid-lincolnshire,Easter, 1905: From April 20th to 26th, 1905     

Henry Preston 《Proceedings of the Geologists' Association. Geologists' Association》1905,19(3):114-IN4

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Excursion to Leicestershire: Whit-Monday,May 21st, 1877, and following day     

Wm. J. Harrison 《Proceedings of the Geologists' Association. Geologists' Association》1877,5(4):142-148

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Dehydration experiments on natural omphacites: qualitative and quantitative characterization by various spectroscopic methods   总被引：1，自引：0，他引：1  

M. Koch-Müller  I. Abs-Wurmbach  D. Rhede  V. Kahlenberg  S. Matsyuk 《Physics and Chemistry of Minerals》2007,34(9):663-678

A series of natural omphacites from a wide range of P, T occurrences were investigated by electron microprobe (EMP), infrared (IR)-, Mössbauer (MS)- and optical spectroscopy in the UV/VIS spectral range (UV/VIS), secondary ion mass spectrometry (SIMS) and single crystal structure refinement by X-ray diffraction (XRD) to study the influence of hydrogen loss on valence state and site occupancies of iron. In accordance with literature data we found Fe²⁺ at M1 as well as at M2, and in a first approach assigned Fe³⁺ to M1, as indicated by MS and XRD results. Hydrogen content of three of our omphacite samples were measured by SIMS. In combination with IR spectroscopy we determined an absorption coefficient: ε _i,tot = 65,000 ± 3,000 lmol_H2O ^?1 cm^?2. Using this new ε _i,tot value, we obtained water concentrations ranging from 60 to 700 ppm H₂O (by weight). Hydrogen loss was simulated by stepwise heating the most water rich samples in air up to 800°C. After heat treatment the samples were analyzed again by IR, MS, UV/VIS, and XRD. Depending on the type of the OH defect, the grade of dehydration with increasing temperature is significantly different. In samples relatively poor in Fe³⁺ (<0.1 Fe³⁺ pfu), hydrogen associated with vacancies at M2 (OH bands around 3,450 cm^?1) starts to leave the structure at about 550°C and is completely gone at 780°C. Hydrogen associated with Al³⁺ at the tetrahedral site (OH bands around 3,525 cm^?1, Koch-Müller et al., Am Mineral, 89:921–931, 2004) remains completely unaffected by heat treatment up to 700°C. But all hydrogen vanished at about 775°C. However, this is different for a more Fe³⁺-rich sample (0.2 Fe³⁺ pfu). Its IR spectrum is characterized by a very intense OH band at 3,515 cm^?1 plus shoulder at 3,450 cm^?1. We assign this intense high-energy band to vibrations of an OH dipole associated with Fe³⁺ at M1 and a vacancy either at M1 or M2. OH release during heating is positively correlated with decrease in Fe²⁺ and combined with increase in Fe³⁺. That dehydration is correlated with oxidation of Fe²⁺ is indirectly confirmed by annealing of one sample in a gas mixing furnace at 700°C under reducing conditions keeping almost constant OH^? content and giving no indication of Fe²⁺-oxidation. Obtained data indicate that in samples with a relatively high concentration of Fe²⁺ at M2 and low-water concentrations, i.e., at a ratio of Fe^{2+ M2}/H > 10 dehydration occurs by iron oxidation of Fe²⁺ exclusively at the M2 site following the reaction: \( {\left[ {{\text{Fe}}^{{{\text{2 + [ M2]}}}}{\text{OH}}^{ - } } \right]} = {\left[ {{\text{Fe}}^{{{\text{3 + [ M2]}}}} {\text{O}}^{{{\text{2}} - }} } \right]} + {\text{1/2}}\;{\text{H}}_{{\text{2}}} \uparrow . \) In samples having relatively low concentration of Fe²⁺ at M2 but high-water concentrations, i.e., ratio of Fe^{2+ M2}/H < 5.0 dehydration occurs through oxidation of Fe²⁺ at M1.  相似文献   

江苏常州4.2级地震前的重力变化     

宋浩  范文华  蒋成  王维  李婷婷  吴晓峰  代宪鹏 《大地测量与地球动力学》2022,42(12):1257-1261

利用江苏地区2019~2021年流动重力观测资料,分析江苏省常州市4.2级地震前不同时间尺度下的重力场变化。结果表明：1）0.5 a尺度重力场变化图像较好地反映了此次地震下降-转折上升-持续上升-反向变化及零值线附近发震的演化过程;2）常州4.2级地震前0.5 a和1 a尺度下的重力场均显示,地震发生在重力变化零值线附近。  相似文献   

M4–18: the planetary nebula and its WC10 central star     

Orsola De Marco  Paul A. Crowther 《Monthly notices of the Royal Astronomical Society》1999,306(4):931-942

We present a detailed analysis of the planetary nebula M4–18 (G146.7+07.6) and its WC10-type Wolf–Rayet (WR) central star, based on high‐quality optical spectroscopy (WHT/UES, INT/IDS, WIYN/DensPak) and imaging ( HST /WFPC2). From a non-LTE model atmosphere analysis of the stellar spectrum, we derive T _eff=31 kK,     v _∞=160 km s⁻¹ and abundance number ratios of H/He<0.5, C/He=0.60 and O/He=0.10. These parameters are remarkably similar to those of He 2–113 ([WC10]). Assuming an identical stellar mass to that determined by De Marco et al. for He 2–113, we obtain a distance of 6.8 kpc to M4–18 [ E ( B−V )=0.55 mag from nebular and stellar techniques]. This implies that the planetary nebula of M4–18 has a dynamical age of ∼3100 yr, in contrast to ≥270 yr for He 2–113. This is supported by the much higher electron density of the latter. These observations may be reconciled with evolutionary predictions only if [WC]-type stars exhibit a range in stellar masses.
Photoionization modelling of M4–18 is carried out using our stellar WR flux distribution, together with blackbody and Kurucz energy distributions obtained from Zanstra analyses. We conclude that the ionizing energy distribution from the WR model provides the best consistency with the observed nebular properties, although discrepancies remain.  相似文献   

UBVI CCD photometry of M35 (NGC 2168)     

H. Sung †  M. S. Bessell † 《Monthly notices of the Royal Astronomical Society》1999,306(2):361-370

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