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21.
以华风集团高清虚拟演播室建设项目为案例,论述了高清虚拟演播室技术在系统建设、系统调试、天气预报节目业务实现环节需要重点解决的几个问题和难点。根据气象电视节目制作要求,在从虚拟演播室系统系统建设到节目制作业务化的整个过程中,重点解决了音频系统延时量计算、绿箱景区施工、绿箱景区灯光布局、绿箱色键抠像调试、摄像机定位与跟踪调试、气象数据调用与转换共6个关键性技术问题。此次业务系统实践的成功是虚拟演播室技术在全国气象影视行业高清节目制作中的应用和推广的很好尝试。 相似文献
22.
最近的多普勒观测表明恒星HD 12661周围存在两颗中等偏心率轨道上运行的行星,内行星的最小质量为2.3木星质量,轨道周期为263.6天;外行星的最小质量为1.57木星质量,轨道周期为1444.5天.该系统的稳定性要求两颗行星处在平运动轨道共振.用数值方法研究了该系统形成初期在恒星气体盘作用下的轨道迁移与稳定性,计算了行星在迁移中被平运动共振俘获的概率.发现这两颗行星目前很可能正处在11:2平运动共振边缘,且运动是混沌的,从而澄清了关于系统目前构形的不同说法,并且很可能在系统形成后行星迁移到目前构形时,气体盘几乎消失了. 相似文献
23.
Frédéric Zagury 《Journal of Astrophysics and Astronomy》2005,26(4):377-394
This paper examines the variations, because of atmospheric extinction, of broad-band visible spectra, obtained from long-slit
spectroscopy, in the vicinity of some stars, nebulae, and one faint galaxy. 相似文献
24.
Our spectroscopic monitoring of the hypergiants HD 168607 (B9.5 Ia-0) and HD 168625 (B5.5 Ia-0) with resolutions from 15000 to 70000 confirms that both stars belong to the Ser OB1 association, proves their spatial closeness, and increases the probability that they constitute a physical pair. 相似文献
25.
Santosh Joshi 《Journal of Astrophysics and Astronomy》2005,26(2-3):193-201
The “Nainital-Cape Survey” program for searching photometric variability in chemically peculiar (CP) stars was initiated in
1997 at ARIES, Nainital. We present here the results obtained to date. The Am stars HD 98851, HD 102480, HD 13079 and HD 113878
were discovered to exhibit δ Scuti type variability. Photometric variability was also discovered in HD 13038, for which the
type of peculiarity and variability is not fully explained. The null results of this survey are also presented and discussed. 相似文献
26.
J. R. Barnes Travis S. Barman L. Prato D. Segransan H. R. A. Jones C. J. Leigh A. Collier Cameron D. J. Pinfield 《Monthly notices of the Royal Astronomical Society》2007,382(1):473-480
We obtained 238 spectra of the close-orbiting extrasolar giant planet HD 189733b with resolution R ∼ 15 000 during one night of observations with the Near-Infrared High-Resolution Spectrograph (NIRSPEC), at the Keck II Telescope. We have searched for planetary absorption signatures in the 2.0–2.4 μm region where H2 O and CO are expected to be the dominant atmospheric opacities. We employ a phase-dependent orbital model and tomographic techniques to search for the planetary absorption signatures in the combined stellar and planetary spectra. Because potential absorption signatures are hidden in the noise of each single exposure, we use a model list of lines to apply a spectral deconvolution. The resulting mean profile possesses a signal-to-noise ratio (S/N) that is 20 times greater than that found in individual lines. Our spectral time series thus yields spectral signatures with a mean S/N = 2720. We are unable to detect a planetary signature at a contrast ratio of log10 ( F p / F * ) =−3.40 , with 63.8 per cent confidence. Our findings are not consistent with model predictions which nevertheless give a good fit to mid-infrared observations of HD 189733b. The 1σ result is a factor of 1.7 times less than the predicted 2.185-μm planet/star flux ratio of log10 ( F p / F * ) ∼−3.16 . 相似文献
27.
Drake Deming † L. Jeremy Richardson Joseph Harrington 《Monthly notices of the Royal Astronomical Society》2007,378(1):148-152
We report infrared photometry of the extrasolar planet HD 209458b during the time of secondary eclipse (planet passing behind the star). Observations were acquired during two secondary eclipses at the NASA Infrared Telescope Facility (IRTF) in 2003 September. We used a circular variable filter (1.5 per cent bandpass) centred at 3.8 μm to isolate the predicted flux peak of the planet at this wavelength. Residual telluric absorption and instrument variations were removed by offsetting the telescope to nearby bright comparison stars at a high temporal cadence. Our results give a secondary eclipse depth of 0.0013 ± 0.0011, not yet sufficient precision to detect the eclipse, whose expected depth is ∼0.002 –0.003 . We here elucidate the current observational limitations to this technique, and discuss the approach needed to achieve detections of hot Jupiter secondary eclipses at 3.8 μm from the ground. 相似文献
28.
R. & R. Griffin 《Journal of Astrophysics and Astronomy》1990,11(3):281-290
HD 201270/1 is a composite-spectrum binary whose components have spectral types close to G8 III and A2 V. They are in a circular
orbit with a period of only 40 days. Photometric variability of RS CVn character is therefore not unlikely 相似文献
29.
30.
J. N. Chkhikvadze 《Astrophysics》2004,47(4):454-461
Spectral and photoelectric (ubvy, H, H) observations of the Herbig Ae/Be star HD 259431 are reported. It is found that as its brightness fades, this star becomes bluer in the Paschen continuum and the intensity and equivalent width of the hydrogen emission lines increase. The spectral observations reveal significant variations in the intensity of the Mg II 4481 Å photospheric absorption line. A rise and fall in the luminosity by 0m.04 within a period of 5-7 minutes was recorded. Radical variations in the H lineshape ("double" "P Cyg") and flare activity are not only observed in this star, but also in a number of HAEBE stars. It is suggested that flare activity may initiate a change in the velocity gradient at the base of the wind and, thereby, induce "double P Cyg" or "P Cyg single" transitions. The nonradial pulsations of this star are also discussed. 相似文献