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301.
A.D. Schwope G. Lamer D. Burke M. Elvis M.G. Watson M.P. Schulze G. Szokoly T. Urrutia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2604-2609
We describe the initial results of a programme to detect and identify extended X-ray sources found serendipitously in XMM-Newton observations. We have analyzed 186 EPIC-PN images at high galactic latitude with a limiting flux of 1 × 10−14 erg cm−2 s−1 and found 62 cluster candidates. Thanks to the enhanced sensitivity of the XMM-Newton telescopes, the new clusters found in this pilot study are on the average fainter, more compact, and more distant than those found in previous X-ray surveys. At our survey limit the surface density of clusters is about 5 deg−2. We also present the first results of an optical follow-up programme aiming at the redshift measurement of a large sample of clusters. The results of this pilot study give a first glimpse on the potential of serendipitous cluster science with XMM-Newton based on real data. The largest, yet to be fulfilled promise is the identification of a large number of high-redshift clusters for cosmological studies up to z = 1 or 1.5. 相似文献
302.
王玉新 《华北航天工业学院学报》2001,11(1):55-56,59
在事物必然的性质、方向和由此决定的活动范围之外,它发生、发展的每一具体变化都是偶然的。为了抓住偶然,就要求助于概率,概率已经成为我们的重要工具。 相似文献
303.
304.
Cool giant and supergiant stars generally present low velocity winds with high mass-loss rates. Several models have been proposed
to explain the acceleration process of these winds. Although dust is known to be present in these objects, the radiation pressure
on these particles is uneffective in reproducing the observed physical parameters of the wind. The most promising acceleration
mechanism cited in the literature is the transference of momentum and energy from Alfvén waves to the gas. Usually, these
models consider the wind to be isothermal. We present a stellar wind model in which the Alfvén waves are used as the main
acceleration mechanism, and determine the temperature profile by solving the energy equation taking into account both the
radiative losses and the wave heating. We also determine, self-consistently, the magnetic field geometry as the result of
the competition between the magnetic field and the thermal pressure gradient. As the main result, we show that the magnetic
geometry presents a super-radial index in the region where the gas pressure is increasing. However, this super-radial index
is greater than that observed for the solar corona. 相似文献
305.
306.
V. Girish V.R. Rana K.P. Singh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2844-2846
We present the analysis of archival Chandra high resolution X-ray spectra of AM Her. Emission lines from several hydrogen-like ions, helium-like ions, Fe-L shell transitions and Fe-K fluorescent are identified. Using the resonance, intercombination and forbidden lines of the few prominent helium-like ions, we infer a density greater than 2 × 1012 cm−3 and a temperature of 2 MK for the oxygen and neon line emitting regions in the accretion column of AM Her. 相似文献
307.
快速成形技术是一种先进的、新型的制造技术,本文介绍了快速成形技术的主要类型和工作过程,并讨论了它在模具制造中的应用。 相似文献
308.
A.J. Blustin G. Branduardi-Raymont E. Behar J.S. Kaastra M.J. Page S.M. Kahn M. Sako K.C. Steenbrugge 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2561-2565
We present results from the analysis of an XMM-Newton observation of the Seyfert 1 galaxy NGC 7469, the first high resolution X-ray spectrum of this source. The Reflection Grating Spectrometer (RGS) spectrum has several narrow absorption and emission lines of O, N, C and Ne, originating from gas at a range of ionisation parameters, from log ξ1.6 to log ξ−2 (where ξ has the units erg cm s−1). We demonstrate that the ionisation state of the warm emitter is consistent with that of the high-ionisation phase of the warm absorber, and compare the warm absorber in this object with those in other sources. 相似文献
309.
本文介绍了30CrMnSiA钢的九种不同的重复热处理工艺,结果显示B种热处理工艺能使30CrMnsiA钢具有最佳的抗疲劳性能并证明不同的重复热处理状态对钢的疲劳性能有影响。 相似文献
310.
A.J. Blustin G. Branduardi-Raymont M.L. Crawford A.A. Breeveld J.S. Kaastra S.M. Kahn 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2540-2543
A large number of galaxies, both normal and active, have been observed in ultraviolet light by the Optical Monitor on XMM-Newton. These are some of the deepest wide-field ultraviolet images of these galaxies yet obtained, and in many cases the first collected in this waveband. We present images of five active galaxies, and discuss the potential uses of the ultraviolet surface brightness distribution and morphology, in association with X-ray data, for Active Galactic Nuclei, star formation and galaxy evolution studies. 相似文献