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61.
C. Simon Jeffery Don Pollacco 《Monthly notices of the Royal Astronomical Society》2000,318(4):974-982
High-speed spectroscopy of two pulsating subdwarf B stars, KPD 2109+4401 and PB 8783, is presented. Radial motions are detected with the same frequencies as reported from photometric observations and with amplitudes of ∼2 km s−1 in two or more independent modes. These represent the first direct observations of surface motion arising from multimode non-radial oscillations in subdwarf B stars. In the case of the sdB+F binary PB 8783, the velocities of both components are resolved; high-frequency oscillations are found only in the sdB star and not the F star. There also appears to be evidence for mutual motion of the binary components. If confirmed, it implies that the F-type companion is ≳1.2 times more massive than the sdB star, while the amplitude of the F-star acceleration over 4 h would constrain the orbital period to lie between 0.5 and 3.2 d. 相似文献
62.
A. Pastorello S. Mattila L. Zampieri M. Della Valle S. J. Smartt S. Valenti I. Agnoletto S. Benetti C. R. Benn D. Branch E. Cappellaro M. Dennefeld J. J. Eldridge A. Gal-Yam A. Harutyunyan I. Hunter H. Kjeldsen Y. Lipkin P. A. Mazzali P. Milne H. Navasardyan E. O. Ofek E. Pian O. Shemmer S. Spiro R. A. Stathakis S. Taubenberger M. Turatto H. Yamaoka 《Monthly notices of the Royal Astronomical Society》2008,389(1):113-130
We present new spectroscopic and photometric data of the Type Ibn supernovae 2006jc, 2000er and 2002ao. We discuss the general properties of this recently proposed supernova family, which also includes SN 1999cq. The early-time monitoring of SN 2000er traces the evolution of this class of objects during the first few days after the shock breakout. An overall similarity in the photometric and spectroscopic evolution is found among the members of this group, which would be unexpected if the energy in these core-collapse events was dominated by the interaction between supernova ejecta and circumstellar medium. Type Ibn supernovae appear to be rather normal Type Ib/c supernova explosions which occur within a He-rich circumstellar environment. SNe Ibn are therefore likely produced by the explosion of Wolf–Rayet progenitors still embedded in the He-rich material lost by the star in recent mass-loss episodes, which resemble known luminous blue variable eruptions. The evolved Wolf–Rayet star could either result from the evolution of a very massive star or be the more evolved member of a massive binary system. We also suggest that there are a number of arguments in favour of a Type Ibn classification for the historical SN 1885A (S-Andromedae), previously considered as an anomalous Type Ia event with some resemblance to SN 1991bg. 相似文献
63.
通过对 2 0 0 0年 1月至 2 0 0 2年 1 2月北京市城市大气污染物SO2 ,PM1 0 ,NO2 的分析发现 :北京市主要污染物是SO2 和PM1 0 。SO2 污染月份主要发生在 1 1月至次年的 3月 ;PM1 03级以上的日数全年都有分布 ,但 4级和 5级的日数主要发生在春季和冬季 ;NO2 主要污染月份发生在 1 0月至次年的 3月 ;大多数污染物以 2 0 0 0年最为严重。对污染资料进行MHAT小波分析发现 ,北京市大气污染存在两个明显的周期波动 ,即 2 0～ 30天周期和准 5天周期 ,这说明北京市污染物浓度短期变化主要受到天气过程及大气低频振荡的影响 ,该文进一步计算了 2 0 0 0年污染资料与气象资料的相关关系发现 ,北京市污染物与日平均气温、日平均风速、每日 1 2 :0 0 (北京时 )温度梯度、相对湿度存在明显的相关关系 ,且不同的气象要素对不同的污染物浓度影响不同。 相似文献