排序方式: 共有38条查询结果,搜索用时 15 毫秒
1.
We present up-to-date evolutionary models of low-mass stars, from M0.6 M down to the hydrogen burning minimum mass, using recent equation of state and synthetic spectra calculations. Comparison is made with observed luminosity function for these objects. We also present implications for the dark-matter distribution in the galactic halo. 相似文献
2.
介绍了采用蓝宝石黑体腔光纤作为传感器的导弹燃气流瞬态温度测量系统的测量原理、系统组成,阐述了其硬件功能模块设计,给出了软件设计算法及蓝宝石黑体腔光纤高温计的标定方法。 相似文献
3.
4.
5.
耐高温有机硅树脂的合成及其耐热和固化性能研究 总被引:29,自引:0,他引:29
以甲基和苯基氯硅烷为单体,采用水解缩聚的方法合成有机硅树脂,并对影响有机硅树脂合成的有关因素进行了研究。结果表明,当水解温度为70℃,控制水用量n(H2O)/n(c1)在8:1-5:1的范围内时,可合成出易溶于甲苯的有机硅树脂。红外光谱(IR)显示,合成的硅树脂含有端羟基。采用热失重法(TG)、热失重的微分曲线法(DTG)和马弗炉烧蚀试验研究有机硅树脂耐的热性能和室温固化性能,并对KH-CL和三乙醇胺两种室温固化剂对硅树脂的耐热性能的影响进行了对比研究。结果表明,在氩气气氛下,硅树脂具有很高的耐热性能,它的起始分解温度为400℃,热失重主要由400-500℃时"解扣式"降解和500℃之后的"重排"降解引起。但在空气气氛下,由于有机基团的氧化分解,硅树脂的耐热性有所下降。KH-CL可使硅树脂在室温条件下固化,固化后硅树脂的耐热性能提高。 相似文献
6.
7.
We describe the formation of hot intergalactic gas along with baryonic remnants in galaxy halos. In this scenario, the mass and metallicity of the hot intracluster and intragroup gas relates directly to the production of baryonic remnants during the collapse of galactic halos. We construct a schematic but self-consistent model in which early bursts of star formation lead to a large remnant population in the halo, and to the outflow of stellar ejecta into the halo and ultimately the Local Group. We consider local as well as high redshift constraints on this scenario. This study suggests that the microlensing objects in the Galactic halo may predominantly be 0.5M white dwarfs, assuming that the initial mass function for early star formation favored the formation of intermediate mass stars with m 1M. However, the bulk of the baryonic dark matter in this scenario is associated with the ejecta of the white dwarf progenitors, and resides in the hot intergalactic medium. 相似文献
8.
Probing the first stars and black holes in the early Universe with the Dark Ages Radio Explorer (DARE) 总被引:1,自引:0,他引:1
Jack O. Burns J. Lazio S. Bale J. Bowman R. Bradley C. Carilli S. Furlanetto G. Harker A. Loeb J. Pritchard 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
A concept for a new space-based cosmology mission called the Dark Ages Radio Explorer (DARE) is presented in this paper. DARE’s science objectives include: (1) When did the first stars form? (2) When did the first accreting black holes form? (3) When did Reionization begin? (4) What surprises does the end of the Dark Ages hold (e.g., Dark Matter decay)? DARE will use the highly-redshifted hyperfine 21-cm transition from neutral hydrogen to track the formation of the first luminous objects by their impact on the intergalactic medium during the end of the Dark Ages and during Cosmic Dawn (redshifts z = 11–35). It will measure the sky-averaged spin temperature of neutral hydrogen at the unexplored epoch 80–420 million years after the Big Bang, providing the first evidence of the earliest stars and galaxies to illuminate the cosmos and testing our models of galaxy formation. DARE’s approach is to measure the expected spectral features in the sky-averaged, redshifted 21-cm signal over a radio bandpass of 40–120 MHz. DARE orbits the Moon for a mission lifetime of 3 years and takes data above the lunar farside, the only location in the inner solar system proven to be free of human-generated radio frequency interference and any significant ionosphere. The science instrument is composed of a low frequency radiometer, including electrically-short, tapered, bi-conical dipole antennas, a receiver, and a digital spectrometer. The smooth frequency response of the antennas and the differential spectral calibration approach using a Markov Chain Monte Carlo technique will be applied to detect the weak cosmic 21-cm signal in the presence of the intense solar system and Galactic foreground emissions. 相似文献
9.
David N. Schramm 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
To illustrate the interaction of Grand Unified Theories (GUTs), supersymmetry (SUSY), and cosmology, a worked example is carried out. This example is the dark matter problem, or “What is the dominant matter of the Universe?” It is shown that if GUTs are assumed then the primordial perturbations are probably adiabatic, if inflation is assumed then Ω = 1 and GUTs first name is probably SUSY. If Ω = 1, big bang nucleosynthesis tells us that the bulk of the matter is non-baryonic. SUSY-GUTs gives us some possible candidate inos to which massive neutrinos, axion or planetary mass black holes can be added. These candidates can be classified hot (or warm) or cold types of dark matter. It is shown that hot gives Ω = 1 and naturally gives large scale structure but does not give small scale structure or galaxy formation times, whereas cold gives small scale structure and formation times but cannot easily yield Ω = 1. It is concluded that either a hybrid of both hot and cold or non-random phases for the perturbations may be needed. 相似文献
10.
检漏间是飞船在航天发射场进行检漏分析的重要设施设备。在对飞船检漏间的基本结构组成进行分析的基础上,建立了基于小孔泄漏模型的飞船检漏间泄漏过程数学模型,并进行了仿真分析。同时,对飞船检漏间迷宫式密封结构的泄漏途径进行了分析,在此基础上,建立了飞船检漏间泄漏因素的故障树模型。依据该模型,通过分析排查试验,明确了泄漏故障发生的具体位置、泄漏原因以及泄漏机理。在采取针对性维修措施的基础上,飞船检漏间漏率指标达到了平均<100Pa/24h的范围,满足了设计指标<150Pa/24h的要求。实际泄漏检测试验表明:上述方法简单、有效。 相似文献