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Qian Shengbang Yang Yuangui Zhu Liying He Jiajia Yuan Jingzhao 《Astrophysics and Space Science》2006,304(1-4):25-28
The formations of the blue straggler stars and the FK Com-type stars are unsolved problems in stellar astrophysics. One of the possibilities for their formations is from the coalescence of W UMa-type overcontact binary systems. Therefore, deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars are a very important source to understand the phenomena of Blue Straggler/FK Com-type stars. Recently, 12 W UMa-type binary stars, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, V410 Aur, XY Boo, SX CrV, QX And, GSC 619-232, and AH Cnc, were investigated photometrically. Apart from TV Mus, XY boo, and GSC 619-232, new observations of the other 9 binaries were obtained. Complete light curves of the 10 systems, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, GSC 619-232, V410 Aur, XY Boo, and AH Cnc, were analyzed with the 2003 version of the W-D code. It is shown that all of those systems are deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars. We found that the system GSC 619-232 has the highest degree of overcontact (f = 93.4%). The derived photometric mass ratio of V857 Her, q = 0.0653, indicates that it is the lowest-mass ratio system among W UMa-type binaries.Of the 12 sample stars, long-term period changes of 11 systems were found. About 58% (seven) of the sample binaries show cyclic period oscillation. No cyclic period changes were discovered for the other 5 systems, which may be caused by the short observational time interval or by insufficient observations. Therefore, we think that all W UMa-type binary stars may contain cyclic period variations. By considering the long-term period changes (both increase and decrease) of those binary stars, we proposed two evolutionary scenarios evolving from deep, low-mass ratio overcontact binaries into Blue Straggler/FK Com-type stars. 相似文献
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The Mt. Suhora M dwarf survey searching for pulsations in low mass main sequence stars has acquired CCD photometry of 46 M dwarf stars during the first year of the project (Baran et al., 2011). As a by-product of this search hundreds field stars have been checked for variability. This paper presents our initial result of a search for periodic variables in field stars observed in the course of the survey. On the basis of the periodicity and the shape of the light curves, eight new variables has been detected, among which five are δ Scuti stars and three likely RR Lyrae stars. Although variation in one of the stars has been previously detected, it was classified incorrectly. To support our classification, in August 2010, we performed spectroscopic observations to derive spectral types and luminosity classes for all eight variable stars. 相似文献
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综合考虑矿物,元素地球化学和孢粉等多方面的资料,对珠江口北岸SX97孔揭示的7000a B.P.以来的气候环境演化提出了一种5阶段划分方案。这种阶段性在SX97孔的各项指标上均有很好的对应,也与华南地区基于海岸沙丘,海滩岩和海相沉积地层等的早期研究成果能较好地对应。在此基础上,初步探讨了气候环境变化中的流域响应,发现SX97孔揭示出气候环境变化中很有很好的流域响应。如当气候环境偏湿偏热时,流域风化作用更加强烈,有很更多的铁元素流失,同时流域植被更发育,对降水有更好的缓冲作用,导致河口沉积物中含有更的铁元素(包括二价铁和三价铁),更少石英矿物和更多粘土矿物,当气候环境偏干偏凉时则相反。 相似文献
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Zdeněk Mikulášek Marek Wolf Miloslav Zejda Petra Pecharová 《Astrophysics and Space Science》2006,304(1-4):363-365
We present two methods for the determination of moments of extrema and their errors appropriate for the analysis of light variations of variable objects. The method I is suitable for determination of times of extrema of non-periodical variables or objects, whose light curves vary. The method II is apt for O-C analyses of objects whose light curves are more or less repeating. Both methods are displayed on the analysis of BL Cam light variations and compared with the Kwee-van Woerden method. 相似文献