C-type shocks in the interstellar medium: profiles of CH⁺ and CH absorption lines     

D. R. Flower  & G. Pineau des Forêts 《Monthly notices of the Royal Astronomical Society》1998,297(4):1182-1188

We have computed optical absorption-line profiles of CH⁺ and CH, as predicted by a model of a C-type shock propagating in a diffuse interstellar cloud. Both these species are produced in the shock wave in the reaction sequence that is initiated by C⁺(H₂, H)CH⁺. Whilst CH⁺ flows at the ion speed, CH, which forms in the dissociative recombination reaction CH⁺₃(e⁻, H₂)CH, flows at a speed which is intermediate between those of the ions and the neutrals. The predicted velocity shift between the CH⁺ and CH line profiles is found to be no more than approximately 2 km s⁻¹, which is smaller than has previously been assumed. We also investigate OH and HCO⁺, finding that the correlation between their column densities, recently observed in the diffuse interstellar medium, can be reproduced by the model.  相似文献   

Gamma-ray bursts: post-burst evolution of fireballs   总被引：3，自引：0，他引：3  

Y. F. Huang  Z. G. Dai  D. M. Wei  & T. Lu 《Monthly notices of the Royal Astronomical Society》1998,298(2):459-463

The post-burst evolution of fireballs that produce γ-ray bursts (GRBs) is studied, assuming the expansion of fireballs to be adiabatic and relativistic. Numerical results as well as an approximate analytic solution for the evolution are presented. Owing to the adoption of a new relation between t R and γ, our results differ markedly from previous studies. Synchrotron radiation from the shocked interstellar medium is carefully calculated, using a conventional set of equations. The observed X-ray flux of GRB afterglows can be reproduced easily. Although the optical afterglows seem much more complicated, our results can still present a rather satisfactory agreement with observations. We also find that the expansion will no longer be highly relativistic about 4 d after the main GRB. We thus suggest that the marginally relativistic phase of the expansion should be investigated so as to check the afterglows observed a week or more later.  相似文献   

Non-axisymmetric relativistic Bondi–Hoyle accretion on to a Schwarzschild black hole     

José A. Font  & J. M. Ibáñez 《Monthly notices of the Royal Astronomical Society》1998,298(3):835-846

We present the results of an exhaustive numerical study of fully relativistic non-axisymmetric Bondi–Hoyle accretion on to a moving Schwarzschild black hole. We have solved the equations of general relativistic hydrodynamics with a high-resolution shock-capturing numerical scheme based on a linearized Riemann solver. The numerical code was previously used to study axisymmetric flow configurations past a Schwarzschild black hole. We have analysed and discussed the flow morphology for a sample of asymptotically high Mach number models. The results of this work reveal that initially asymptotic uniform flows always accrete on to the hole in a stationary way, which closely resembles the previous axisymmetric patterns. This is in contrast with some Newtonian numerical studies where violent flip-flop instabilities were found. As discussed in the text, the reason can be found in the initial conditions used in the relativistic regime, as they cannot exactly duplicate the previous Newtonian setups where the instability appeared. The dependence of the final solution on the inner boundary condition as well as on the grid resolution has also been studied. Finally, we have computed the accretion rates of mass and linear and angular momentum.  相似文献   

Double detonations at the core–envelope boundary in Type Ia supernovae     

D. J. R. Wiggins  G. J. Sharpe  & S. A. E. G. Falle 《Monthly notices of the Royal Astronomical Society》1998,301(2):405-413

An off-centre detonation propagating near the interface between a C–O core and a He envelope in a Type Ia supernova explosion is modelled as a steady two-dimensional similarity solution at a plane interface. We assume that in both regions the energy release occurs in an infinitely thin detonation, which produces material in nuclear statistical equilibrium (NSE) in He and in nuclear statistical quasi-equilibrium in C–O. An α-network is then used to determine the effect of the associated rarefaction wave in the C–O on the final abundance of intermediate elements. We find that, although there is a significant effect, the rarefaction is not strong enough to quench the reactions and prevent the C–O from burning to NSE.  相似文献   

Expression of heat shock protein 70 in a permanent cell line (EPC) exposed to sediment extracts from the North Sea and the Baltic Sea     

Kinder A  Sierts-Herrmann A  Biselli S  Heinzel N  Hühnerfuss H  Kammann U  Reineke N  Theobald N  Steinhart H 《Marine environmental research》2007,63(5):506-515

Heat shock proteins 70 (hsp70) are known to be induced by a great variety of chemical stressors. The effects of different environmental contaminants, which were identified in sediments of the North Sea and the Baltic Sea as main contaminants or as contaminants of special toxicological interest, on the extent of expression of hsp70 in a permanent cell line Epithelioma papulosum cyprini (EPC) were investigated. Concentrations of the single contaminants leading to elevated hsp70 levels were compared to the respective concentrations of these contaminants encountered in the sediment extracts thus allowing an assessment of their contribution to the toxicity of these sediments. Analysis of hsp70 was performed using western blotting techniques with subsequent comparative quantification by densitometry. Eleven of thirteen contaminants have shown a dose-dependent increase in hsp70 levels. An expression of hsp70 was observed in most cases between 0.1 and 10 microg/mL test solution. Some of the investigated stressors led to extremely high hsp70 contents even at low concentrations. However, in most cases contaminant concentrations in sediments were too low to cause an effect. For this reason, effects of the tested sediments are attributed to other contaminants or rather to mixtures of stressors.  相似文献   

真鲷三倍体诱导初步研究     

蔡国雄 《热带海洋学报》1997,(4)

在真鲷Pagrosomusmajor三倍体诱导研究中，对染色体倍数的分析表明，受精卵受精5min后，在1．5℃冰水中处理5min，可获得17％的三倍体诱导率和28％的嵌合体比率，染色体数分别是：2N＝48，3N＝7Z，嵌合体50—68。仔鱼红血细胞测量和组织切片分析显示，三倍体和二倍体的红血细胞核直径（长径，下同）、视网膜神经节细胞核直径和中脑细胞核直径大小存在差异，其比率分别是1．42，1．35和1．41，这种差别必然导致三倍体鱼和二倍体鱼在代谢与功能方面的差异。应加强对鱼类三倍体形成机制及应用潜力的研究，同时注意开展其生理学、生化学和行为学的比较研究。  相似文献   

Tetraploid induced by physical and chemical methods in Jinjiang oyster(Crassostrea rivularis)   总被引：1，自引：0，他引：1  

Rong Shoubai  Shi Shumei  Mo Qirong  Liu Shaeqiong  Liang Ze  Zhao Xiuzhu  Tong Wangdong  Li Shouwu  Li Yimin 《海洋学报(英文版)》1994,13(2):275-283

ＴｅｔｒａｐｌｏｉｄｉｎｄｕｃｅｄｂｙｐｈｙｓｉｃａｌａｎｄｃｈｅｍｉｃａｌｍｅｔｈｏｄｓｉｎＪｉｎｊｉａｎｇｏｙｓｔｅｒ（Ｃｒａｓｓｏｓｔｒｅａｒｉｖｕｌａｒｉｓ）￥ＲｏｎｇＳｈｏｕｂａｉ，ＳｈｉＳｈｕｍｅｉ，ＭｃＱｉｒｏｎｇ，ＬｉｕＳｈａｅｑｉｏ...  相似文献   

华贵栉孔扇贝三倍体的研究   总被引：2，自引：1，他引：2  

曾志南  陈木等 《台湾海峡》1995,14(2):155-162

本文报道了用细胞松驰素B、高温和低温休克等方法诱导华贵栉孔扇贝（Chlamys nobilis）三倍体的实验结果。在26.0～28.0℃条件下，选用不同浓度的细胞松驰素B0.1、0.3、0.5、0.7和1.0mg/dm^3，在受精后15min，处理受精卵15min，三倍体诱导率分别为12.5%、37.5%、68.0%、66.6%和81.0%，其中0.5～1.0mg/dm^3浓度的细胞松驰素B对改变倍性最有效。高温休克选用31.0、33.0、35.0和37.0℃处理受精卵，最高三倍体诱导率达46.7%（33.0℃,处理15min）。低温休克选用6.0、8.0、10.0和12.0℃处理受精卵，最高三倍体诱导率为40.7%（10.0℃，处理20min）。实验结果表明，随着处理强度的增大和处理时间的延长，三倍体诱导率增高、但孵化率下降，畸型率上升。用高温休克处理的实验组幼虫生长速度较对照组快。作者认为，在商业性生产中，温度休克是诱导扇贝三倍体的一种简便、有效的方法。文中还就细胞松驰素B与温度休克诱导三倍体的机制进行了讨论。  相似文献   

Astrophysical boosters     

W. Kundt 《Journal of Astrophysics and Astronomy》1984,5(3):277-283

Constraints are derived on the acceleration of charges in shocks to highly relativistic energies. When applied to the extended extragalactic radio sources and to the cosmic rays, they cast doubt on the mechanism of ‘in-situ acceleration’, both for energy, entropy and statistical mechanics reasons.  相似文献   

Relativistic Fermi acceleration with shock compressed turbulence     

Martin Lemoine  Benoît Revenu 《Monthly notices of the Royal Astronomical Society》2006,366(2):635-644

  相似文献