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1.
We report three new or updated techniques for probing the parameters of active galaxies based on the masses of their central
black holes MBH). First, we derived a near-IR analog of the bulge luminosity versus MBH relationship. The low scatter makes it a promising new tool to study the black hole demographics. Next, we present relations
between MBH and the10 μm and 2-10 keV nuclear luminosity. They may help to study the MBH evolution over wide redshift ranges. Finally, we measured MBH in quasars from z ∼ 3.4 to z ∼ 0.3 to search directly for MBH growth. Surprisingly, we found no evidence for growth implying that the majority of quasar host galaxies have undergone their
last major merger at z ≥ 3.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
2.
The lensing properties of the Plummer model with a central point mass and external shear are derived, including the image multiplicities, critical curves and caustics. This provides a simple model for a flattened galaxy with a central supermassive black hole. For the Plummer model with black hole, the maximum number of images is four, provided the black hole mass is less than an upper bound which is calculated analytically. This introduces a method to constrain black hole masses by counting images, thus applicable at cosmological distance. With shear, the maximum number of images is six and we illustrate the occurrence of an astroid caustic and two metamorphoses. 相似文献
3.
沙文生 《云南地理环境研究》2004,(Z1)
利用2004年5月15~21日第一场透雨过程的高空资料,对产生强降雨天气的主要物理量进行分析,总结主要物理量的变化特征,揭示这次强降雨产生发展变化规律,对今后在预报过程中对主要物理量的变化引起重视,具有一定的参考意义。 相似文献
4.
The high-altitude dayside cusps (both northern and southern) are extremely dynamic regions in geospace. Large diamagnetic cavities with significant fluctuations of the local magnetic field strength have been observed there. These cusp diamagnetic cavities are always there day after day and are as large as 6 RE Associated with these cavities are charged particles with energies from 20 keV up to 10 MeV. The intensities of the cusp energetic ions have been observed to increase by as much as four orders of the magnitude when compared with regions adjacent to the cusp which includes the magnetosheath. Their seed populations are a mixture of ionospheric and solar wind particles. The measured energetic ion fluxes in the high-altitude cusp are higher than that in both the regions upstream and downstream from the bow shock. Turbulent electric fields with an amplitude of about 10 mV/m are also present in the cusp, and a cusp resonant acceleration mechanism is suggested. The observations indicate that the dayside high-altitude cusp is a key region for transferring the solar wind mass, momentum, and energy into the Earth’s magnetosphere. 相似文献
5.
Wei Yong Rong Zhaojin Zhong Jun Chai Lihui Yue Xin an Liu Libo Yu Sheng Zhu Rixiang Wan Weixing 《地球科学进展》2017,32(1):15-20
It has been 60 years since the space physics as new branch of geophysics started to grow in 1957 when the space age was opened by a small satellite called sputnik. The knowledge of Earth and planetary space has been significantly extended and deepened, but the questions we are facing today are more challenging. A consensus reached is that we have to regard the Earth (planet) as an integrated system including all spheres from the inner core to the magnetosphere, and we should try to investigate some questions standing on the ground of interdisciplinary study, especially those questions related to Earth’s (planetary) evolution. Space environment as the outer part of a planetary system, commonly exists in all planets but also exhibits strong diversity. Here, we introduce the short history of basic ideas and methods of comparative study, the advantages on understanding of some issues of global scale, and the prospect from comparative perspective. 相似文献
6.
西北地区春季云系的垂直结构特征飞机观测统计分析 总被引:11,自引:0,他引:11
根据2001年5—6月8架次的飞机探测资料,配合地面观测和卫星资料综合分析得出了西北地区春季云系的垂直结构宏微观特征,包括云厚、云底高度、云粒子浓度、含水量、有效半径、粒子谱分布函数等。降水性层状云厚平均约2000 m,低云含水量垂直方向上平均为0.07 g·m~(-3),中云含水量垂直方向上平均为0.03 g·m~(-3)。对比分析降水云和非降水云系的微物理特征量,两者存在显著的差异,降水性层状云有效半径要达到10~16μm。 相似文献
7.
玻色-爱因斯坦凝聚和重力测量——2001年诺贝尔物理学奖评介 总被引:6,自引:0,他引:6
介绍了2001年诺贝尔物理学奖获得者康奈尔,韦曼,克特勒的科学研究成果,实验玻色-爱因斯坦凝聚(BEC)及其在理论上的意义和应用前景,讨论了BEC在研制高精度重力仪方面的应用问题,为此回顾了重力测量现状,朱棣文等研制的原子干涉重力仪和ClauserJ提出的物质波干涉重力仪,分析表明,如果利用BEC,则重力仪的测量精度在朱棣文等工作基础上将会有很大的提高。 相似文献
8.
9.
Gerald Schubert 《天文和天体物理学研究(英文版)》2019,(4):7-22
With a great deal of humility I attempt in the following to recall important events in my life and in my scientific career of more than five decades. I am not through yet. I continue to do research though, I admit, not with the energy and fervor I once had. Still, I hope to contribute to science in meaningful ways. 相似文献
10.
Yan Yan 《天文和天体物理学研究(英文版)》2019,(5):101-112
We investigate the masses of glitching pulsars in order to constrain their equation of state(EOS). The observations of glitches(sudden jumps in rotational frequency) may provide information on the interior physics of neutron stars. With the assumption that glitches are triggered by superfluid neutrons, the masses of glitching neutron stars can be estimated using observations of maximum glitches.Together with the observations of thermal emission from glitching pulsars Vela and J1709–4429, the slope of symmetry energy and incompressibility of nuclear matter at saturation density can be constrained.The slope of symmetry energy L should be larger than 67 MeV while the lower limit of incompressibility for symmetric nuclear matter K_0 is 215 MeV. We also obtain a relationship between L and K_0:6.173 MeV + 0.283 K_0≤ L ≤ 7.729 MeV + 0.291 K_0. The restricted EOSs are consistent with the observations of 2-solar-mass neutron stars and gravitational waves from a binary neutron star inspiral. 相似文献