Short-period AM CVn systems as optical, X-ray and gravitational-wave sources   总被引：1，自引：0，他引：1  

G. Nelemans  L. R. Yungelson  S. F. Portegies Zwart 《Monthly notices of the Royal Astronomical Society》2004,349(1):181-192

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A new interpretation of the remarkable X-ray spectrum of the symbiotic star CH Cyg     

Peter J. Wheatley  Timothy R. Kallman 《Monthly notices of the Royal Astronomical Society》2006,372(4):1602-1606

We have re-analysed the ASCA X-ray spectrum of the bright symbiotic star CH Cyg, which exhibits apparently distinct hard and soft X-ray components. Our analysis demonstrates that the soft X-ray emission can be interpreted as scattering of the hard X-ray component in a photoionized medium surrounding the white dwarf. This is in contrast to previous analyses in which the soft X-ray emission was fitted separately and assumed to arise independently of the hard X-ray component. We note the striking similarity between the X-ray spectra of CH Cyg and Seyfert 2 galaxies, which are also believed to exhibit scattering in a photoionized medium.  相似文献   

On the evolution of the nova-like variable AE Aquarii     

P. J. Meintjes 《Monthly notices of the Royal Astronomical Society》2002,336(1):265-275

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1991年10月24日白光耀斑的高时间分辨率多波段光谱分析     

周曦  方成  胡菊 《中国天文和天体物理学报》1996,(4)

本文分析了南京大学太阳塔1991年10月24日用多波段光谱仪观测到的高时间分辨率（5s）的一个2N／X2．1级白光耀斑光谱．对耀斑谱线轮廓、连续发射强度、X射线和射电爆发资料进行了综合对比，分析表明，该耀斑属Ⅰ类白光耀斑，具有如下特征：（1）在白光耀斑的脉冲相期间，各波段光谱线心强度、连续辐射、谱线半宽以及线翼红不对称性与硬X射线高能波段的爆发同时达到极大；（2）H_a谱线在连续发射极大时半宽达10A，且呈现强烈的线心反转，H_β和H_γ线心亦有反转；（3）所拍摄的5条谱线都有明显的红不对称性，持续时间约为1分钟，根据上述结果，本文用电子束轰击、色球蒸发和色球压缩区对该耀斑能量积聚和释放的动力学机制作了定性的分析和解释。  相似文献   

Hidden subluminous stars among the FAUST UV sources towards Ophiuchus     

Liliana Formiggini  Noah Brosch  Elchanan Almoznino  Stuart Bowyer  Michael Lampton 《Monthly notices of the Royal Astronomical Society》2002,332(2):441-455

We present results of an analysis of a UV image in the direction of Ophiuchus, obtained with the FAUST instrument. The image contains 228 UV sources. Most of these are identified as normal early-type stars through correlations with catalogued objects. For the first time in this project we identify UV sources as such stars by selecting suitable candidates in crowded fields as the bluest objects in colour–colour diagrams using observations from the Wise Observatory. These candidates are then studied using low-resolution spectroscopy, which allows the determination of spectral types to an accuracy of about one-half class, for 60 stars.
Synthetic photometry of spectral data is performed in order to predict the expected UV emission, on the basis of the photometric information. These results are used along with the Hipparcos /Tycho information, to search for subluminous stars. The comparison of the predicted emission with the FAUST measured magnitudes allows us to select 12 stars as highly probable evolved hot stars. High signal-to-noise spectra are obtained for nine of these stars, and Balmer line profiles are compared with the prediction of atmosphere models and with the spectrum of real stellar atmospheres. Among the nine candidates, six are classified as previously unrecognized sdB stars, and two as white dwarfs. Our result indicates that indeed more bright subluminous stars are still unrecognized in the existing samples.  相似文献   

Improved synthetic spectra of helium-core white dwarf stars     

R. D. Rohrmann  †‡  A. M. Serenelli  §  L. G. Althaus ¶  O. G. Benvenuto &#; 《Monthly notices of the Royal Astronomical Society》2002,335(2):499-511

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Type Ia supernovae and remnant neutron stars     

A. R. King  J. E. Pringle  D. T. Wickramasinghe 《Monthly notices of the Royal Astronomical Society》2001,320(3):L45-L48

On the basis of the current observational evidence, we put forward the case that the merger of two CO white dwarfs produces both a Type Ia supernova explosion and a stellar remnant, the latter in the form of a magnetar. The estimated occurrence rates raise the possibility that many, if not most, Type Ia supernovae might result from white dwarf mergers.  相似文献   

激变变星中的快速光变   总被引：2，自引：0，他引：2  

李宗云  丁月蓉 《天文学进展》1996,14(2):139-148

文中综述了激变变星中快速光变的研究进展，讨论了闪变，相干振荡和准周期振荡的观测特征和可能的产生机制。  相似文献   

山岳型景区建设下乡村聚落的多维重构——基于云丘山旅游景区微观案例的实证研究   总被引：1，自引：0，他引：1  

朱鹤  刘家明 《地理研究》2018,37(12):2490-2502

随着乡村旅游的快速发展,传统乡村发生了巨大变化,尤其在山区地区,受自然环境、资源条件的影响,其乡村聚落的重构更具有独特性和典型性。采取深度访谈、全样本问卷调查、遥感影像解译与GIS分析等方法,以云丘山旅游景区中的两个自然村落为例,从微观尺度研究乡村聚落的多维重构过程,研究发现,在景区建设推动下,云丘山景区内两个村的“空间—经济—社会”三个维度均发生了重构：空间层次上,土地利用状况和三生空间的规模均发生变化,生产、生活空间减少,生态空间增加,空间格局上从“生活—生产—生态”的环状模式转变为生活、生产空间在生态空间中镶嵌的模式;经济层次上,村民的收入提升,生计模式发生改变,对旅游业的产业依赖度升高,传统生产模式改变;社会层次上,人口回流,劳动力显著增加,社会阶层的空间差异被打破,乡村组织方式逐渐向旅游生产方式上转变。乡村的“空间—经济—社会”多维重构之间存在相互影响关系,在景区旅游发展的推动下形成新的乡村地域系统。  相似文献   

Optimization of spatial statistical approaches to identify land use/land cover change hot spots of Pune region of Maharashtra using remote sensing and GIS techniques     

Kuntal Ganguly  Rajiv Kumar  K. Mruthyunjaya Reddy  P. Jagadeeswara Rao  Manoj Raj Saxena  G. Ravi Shankar 《国际地球制图》2017,32(7):777-796

This study investigated land use/land cover change (LULCC) dynamics using temporal satellite images and spatial statistical cluster analysis approaches in order to identify potential LULCC hot spots in the Pune region. LULCC hot spot classes defined as new, progressive and non-progressive were derived from Gi* scores. Results indicate that progressive hot spots have experienced high growth in terms of urban built-up areas (20.67% in 1972–1992 and 19.44% in 1992–2012), industrial areas (0.73% in 1972–1992 and 3.46% in 1992–2012) and fallow lands (4.35% in 1972–1992 and ?6.38% in 1992–2012). It was also noticed that about 28.26% of areas near the city were identified as new hot spots after 1992. Hence, non-significant change areas were identified as non-progressive after 1992. The study demonstrated that LULCC hot spot mapping through the integrated spatial statistical approach was an effective approach for analysing the direction, rate, spatial pattern and spatial relationship of LULCC.  相似文献