成藏过程对天然气地球化学特征的控制作用   总被引：3，自引：0，他引：3  

赵孟军  潘文庆  张水昌  韩剑发 《沉积学报》2004,22(4):683-688

克拉2和阿克1天然气都具有组分明显偏干、碳同位素明显偏重的特征,如克拉2和阿克1天然气的干燥系数都接近于1.0,克拉2天然气的δ13C₁为-27.3‰～-31.1‰,阿克1天然气的δ13C₁为-21.9‰～-25.2‰,从“源控”的角度似乎这些天然气应该属于过成熟煤成气,这样计算所得到的天然气成熟度远大于实测和模拟计算的源岩成熟度。因此在解释克拉2和阿克1天然气数据的时候,除了“源控”的因素外,更应强调成藏过程的影响。分析认为晚期阶段聚气是造成克拉2和阿克1天然气都具有组分明显偏干、碳同位素明显偏重的主要因素。  相似文献   

Results from multifrequency observations of PSR B0826−34     

B. Bhattacharyya  Y. Gupta  J. Gil 《Monthly notices of the Royal Astronomical Society》2008,383(4):1538-1550

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Are ring galaxies the ancestors of giant low surface brightness galaxies?     

M. Mapelli  B. Moore  E. Ripamonti  L. Mayer  M. Colpi  L. Giordano 《Monthly notices of the Royal Astronomical Society》2008,383(3):1223-1231

We simulate the collisional formation of a ring galaxy and we integrate its evolution up to 1.5 Gyr after the interaction. About 100–200 Myr after the collision, the simulated galaxy is very similar to observed ring galaxies (e.g. Cartwheel). After this stage, the ring keeps expanding and fades. Approximately 0.5–1 Gyr after the interaction, the disc becomes very large (∼100 kpc) and flat. Such extended discs have been observed only in giant low surface brightness galaxies (GLSBs). We compare various properties of our simulated galaxies (surface brightness profile, morphology, H  i spectrum and rotation curve) with the observations of four well-known GLSBs (UGC 6614, Malin 1, Malin 2 and NGC 7589). The simulations match quite well the observations, suggesting that ring galaxies could be the progenitors of GLSBs. This result is crucial for the cold dark matter (CDM) model, as it was very difficult, so far, to explain the formation of GLSBs within the CDM scenario.  相似文献   

Daily observations of interstellar scintillation in PSR B0329+54     

N. Wang  Z. Yan  R. N. Manchester  H. X. Wang 《Monthly notices of the Royal Astronomical Society》2008,385(3):1393-1401

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Geometry of Broad Line Regions of Active Galactic Nuclei     

Xiao-Rong Lu 《天体物理学报》2008,8(1):50-62

It has long remained an open question as to the geometry of the broad line region （BLR） in active galactic nuclei （AGNs）. The reverberation mapping technique which measures the response of the broad emission lines to the ionizing continuum, when combined with multiwavelength continuum fitted by sophisticated accretion disks, provides a way of probing the BLR geometry. We analyze a sample of 35 AGNs, which have been monitored by the reverberation mapping campaign. In view of energy budget, the reverberation-based BH masses are found to be in agreement with those obtained by accretion disk models in two thirds of the present sample while the reverberation mapping methods underestimate the BH masses in about one third of objects, as also suggested by CoUin et al. in a recent work. We point out that there are obviously two kinds of BLR geometry, which are strongly dependent on the Eddington ratio, and separated by the value LBol/LEdd - 0.1. These results prefer a scenario of the disk and wind configuration of the BLR and identify the Eddington ratio as the physical driver regulating the wind in the BLR.  相似文献   

Possible Contribution of Mature γ-ray Pulsars to Cosmic-ray Positrons     

Quan-Gui Gao Ze-Jun Jiang Li Zhang 《天体物理学报》2008,8(1):87-95

We restudy the possible contribution of mature gamma-ray pulsars to cosmic ray positrons based on the new version of outer gap model. In this model, the inclination angle and average properties of the outer gap are taken into account, and more mature pulsars can have the outer gap and emit high energy photons. Half of the primary particles in the outer gaps will flow back toward the star surface and emit synchrotron photons, which can produce electron/positron pairs by the cascade of pair production. Some of these pairs will escape from the light cylinder and be accelerated to relativistic energies in the pulsar wind driven by low-frequency electromagnetic waves. Using a Monte Carlo method, we obtain a sample of mature gamma-ray pulsars and then calculate the production of the positrons from these pulsars. The observed excess of cosmic positrons can be well explained by this model.  相似文献   

Growth of Black Holes and Their Host Spheroids in （Sub）mm-loud High-Redshift QSOs     

Cai-Na Hao Xiao-Yang Xia Shu-De Mao Zu-Gan Deng Hong Wu 《天体物理学报》2008,8(1):12-24

We study the growth of black holes and stellar population in spheroids at high redshift using several （sub）mm-loud QSO samples. Applying the same criteria established in an earlier work, we find that, similar to IR QSOs at low redshift, the far-infrared emission of these （sub）mm-loud QSOs mainly originates from dust heated by starbursts. By combining low-z IR QSOs and high-z （sub）mm-loud QSOs, we find a trend that the star formation rate （M＊） increases with the accretion rate （Mace）. We compare the values of M＊/Macc for submm emitting galaxies （SMGs）, far-infrared ultraluminous/hypeduminous QSOs and typical QSOs, and construct a likely evolution scenario for these objects. The （sub）mm-loud QSO transition phase has both high Macc and M＊ and hence is important for establishing the correlation between the masses of black holes and spheroids.  相似文献   

Star-Forming Galaxies at z～2 in the Hubble Ultra Deep Field     

《中国天文和天体物理学报》2008,8(1):1-11

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Correlated Radio-Optical Variations on Intraday Timescales     

Shan-Jie Qian 《中国天文和天体物理学报》2008,8(2):219-229

Correlated radio-optical variations on intraday timescales have been observed (e.g. In BLO 0716 714) and such radio intraday variability is suggested to have an intrinsic ori- gin. Recently, multi-wavelength observations, simultaneous at radio, mm-submm, optical and hard X-rays, of 0716 714, show that during a period of intraday/interday variations at ra- dio and mm wavelengths, the apparent brightness temperature of the source exceeded the Compton-limit (～1012 K) by 2--4 orders of magnitude, but no Compton catastrophe (or no high luminosity of inverse-Compton radiation) was detected. It is also found that the intra- day/interday variations at mm-submm wavelengths are consistent with the evolutionary be- havior of a standard synchrotron source and for the intraday/interday variations at centimeter wavelengths opacity effects can play a significant role, which is consistent with the interpreta- tion suggested previously by Qian et al. Thus the apparent high brightness temperatures may probably be explained in terms of Doppler boosting effects due to bulk relativistic motion of the source. We will argue a scenario to simulate the correlations between the radio and optical variations on intraday timescales observed in BLO 0716 714 in terms of a relativistic shock propagating through a jet with a dual structure.  相似文献   

Detection of CO Outflow in Rotating Cores     

Xin Guan  Yue-Fang Wu 《中国天文和天体物理学报》2008,8(2):230-236

We investigate the effect of bulk motion on the detection of molecular outflows in the sources S 146, GGD27, and IRAS 22566 5830. The traditional techniques do allow for bulk motions or systematic VLSR shifts of the core emissions, which may cause contamination of the high velocity gas emissions, and outflows may either fail to be detected or have their properties miscalculated. We used a program to follow the systematic shift of VLSR and better results have been obtained.  相似文献