排序方式： 共有47条查询结果，搜索用时 15 毫秒
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Klochkova V. G. Panchuk V. E. Tavolzhanskaya N. S. Yushkin M. V. 《Astronomy Letters》2020,46(8):528-540
Astronomy Letters - Evidence of wind variability and velocity stratification in the extended atmosphere has been found in the spectra of the supergiant V340 Ser ( $${=}$$ IRAS 17279 $$-$$ 1119)... 相似文献
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The optical layout and performance characteristics of a device for measuring the four Stokes parameters are reported, and the principle of its operation is described. The device is designed for use in the NES echelle spectrograph mounted in the Nasmyth-2 focus of the 6-meter telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. Tests of the device operating on the telescope showed the gain in throughput to be a factor of 2.7 and 6 in the red (5000–7000 Å Å) and blue (3500–4700 Å Å) parts of the spectrum, respectively, compared to an analyzer based on Fresnel rhombi. 相似文献
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Valentina G. Klochkova Eugene L. Chentsov Tonu Kipper Vladimir E. Panchuk Nonna S. Tavolganskaya Maxim V. Yushkin 《Astrophysics and Space Science》2011,335(1):83-89
We present a spectral atlas of 4 B and A stars containing spectra in a poorly studied spectral range of 305–452 nm. The atlas
is based on high resolution (R=60 000) spectra obtained with the 6 meter telescope (SAO, Russia) combined with the NES-spectrograph. The procedure of spectral
lines identification and compilation of the atlas is discussed in detail. Using the spectral data we thoroughly investigated
the velocity field in expanding atmospheres and envelopes of hot evolved stars β Ori, α Cyg and supergiant KS Per with the extreme hydrogen deficiency. The complete atlas and list of the identified spectral lines
will be available via the astronomical database SIMBAD. 相似文献
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The potential of an algorithm of semiempirical modeling of stellar spectra recorded via an iodine absorption cell is analyzed. This algorithm, when used with the NES quartz echelle spectrograph of the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences, is shown to be able to achieve a Doppler shift measurement accuracy of 20 m/s with an internal accuracy of 2 m/s. 相似文献
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生物和矿物体系的结构、功能和演化的比较分析与生物有机体中生命矿物的功能令人对生物世界矿物根的存在产生了怀疑。文章提出,应在非生物成因有序碳氢分子体系（硬沥青）中寻找前生物信息结构、基因之祖和原生有机体。前生物有机体的理想模型是纤维状黄绿蛭石,它是按照ＶＬＳ机制在伟晶岩的孔洞中结晶出来的,其形态、结构和成分与生物有机体十分相似。生命世界不是矿物世界转化的产物。生命世界和矿物世界都有共同的来源———非紧密离子分子体系,在该体系中,它们相互和谐作用,以不同的结晶机理发生和发展。生命作为统一的整体,作为复杂碳氢体系结晶作用的完整结果产生和演化,而不是偶然事件巧合或不同成因组分结合的结果。矿物和生物有机体的演化受控于共同的个体发生律。根据纤维状黄绿蛭石晶体的研究而提出的晶质原生有机体模型,消除了在创立统一的自然发生论概念（结构组织、大分子集合、继承机理、手性选择等等）方面的主要分歧和障碍。这就使把解决生命起源问题带入实验模拟层次成为现实 相似文献
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D. R. Gadelshin G. G. Valyavin M. V. Yushkin E. A. Semenko G. A. Galazutdinov O. V. Maryeva A. F. Valeev Byeong-Cheol Lee 《Astrophysical Bulletin》2017,72(3):330-336
We present the results of spectroscopic confirmation of exoplanet candidates from the “Kepler” space mission catalog. We used the NES spectrometer of the 6-m Russian BTA telescope to investigate the Doppler variability of the radial velocities of the host stars of KOI-974.01, KOI-2687.01/02, and KOI-2706.01. According to the derived upper limits, KOI-2706.01 has a mass significantly smaller than 12 Jupiter masses, which directly indicates its planetary nature. We show that KOI-2687.01 and KOI-2687.02, which have Earth-size or white dwarf-size radii according to photometric data, cannot be white dwarfs, and are therefore exoplanets. Radial velocity analysis for KOI-974, an F-type star, has shown noticeable variations with a half-amplitude of 400 ms?1, which correlate poorly with the phase of its orbital rotation. This can indicate a presence of other massive planets in the system, with orbits closer or farther from the host star than the orbit of KOI-974.01, or a low mass star in a distant outer orbit. Using the method of synthetic spectra, we obtained more accurate atmospheric parameter and radius estimates for all the program host stars, which, in turn, allowed us to refine the radii of the studied exoplanet candidates. 相似文献
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We report an efficient method for analyzing the radial-velocity and line-profile variability. We show that a detailed analysis of the variations of line profiles and velocity field in the stellar atmosphere requires the radial velocities to be measured separately for the blue and red halves of the absorption lines at different levels of their residual intensity. We applied this method to 120 CCD spectra taken in 1998–99 with the coude echelle spectrograph attached to the 2-m telescope of Shemakha Astronomical Observatory of National Academy of Sciences of Azerbaijan and analyzed the variations of the radial velocities and profiles of ion and Hβ lines in the spectrum of α Cyg. In the case of ion lines both halves of the absorption profile exhibit synchronous radial-velocity variations at all levels of line intensity. In the case of the Hβ line, which forms in the layers where stellar wind originates, the pattern of radial-velocity variations differs for the blue and red halves of the absorption profile. The variability pattern is the same at all levels in the red half of the profile, the blue half of the profile exhibits different variability patterns at different levels of residual line intensity. Identification and analysis of such variations allows us to study the nature of stellar-wind variability in the region of wind formation.The spectrum of α Cyg showed no line-profile or radial-velocity variations for six days in both halves of the absorption contour at all levels of line intensity. The star was in the quiescent phase. 相似文献