X-ray activity cycles

来源 :第二届太阳系外行星系统的发现和刻画国际研讨会(The Second Workshop for Exoplanetary | 被引量 : 0次 | 上传用户:vingf
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
Outline Examples of X-ray cycles:Tau Boo,HD 81809,61 Cyg A,α Cen A&B HR 1099/V711 Tau:Circumbinary planet or activity?
其他文献
Outline · KM2A:The high energy detector of LHAASO (10 TeV-1 PeV) · Simulation of KM2A · Choice of a fast simulation · Structure of the simulation
会议
Motivation:We measure directly the spectra of Cosmic Rays only for:a single point in the Galaxy [the solar system] and a unique time (the present).
会议
Content ·1.Introduction about LHAASO ·2.Status of LHAASO software ·2.1 Status of WCDA ·2.2 Status of WCDA++·2.3 Status of KM2A ·2.4 Status of WFCTA ·3.Status of LHAASO framework and future plan ·4.Sum
会议
The Yangbajing Cosmic Ray Laboratory Tibet-China The ARGO-YBJ detector Single layer of RPCs detectors · Central carpet 78 × 75 m2 (95% of active surface)
会议
Content ·Status and difficulties in cosmic ray measurements ·Introduction of direct Cherenkov light ·Monte Carlo study based on LHAASO-WFCTA ·Improvement of the discrimination of heavy cosmic rays by
会议
Tidal disruption event (TDE) 101 (Komossa 15 review) Figures from Rees 1988 Theory:· Inevitable:galaxies have supermassive black holes
会议
Recent precise measurements of cosmic-ray(CR)spectra show that the energy distribution of protons is softer than those of heavier nuclei,and there are spectral hardenings for all nuclear compositions
Outline Introduction Chromospheric activity Stellar prominence Stellar activity and Exoplanet Some of our research works
会议
PLANETS AND THEIR LIGHT CURVES SECONDARY TRANSITS(OCCULTATIONS)and the orbit parameters
会议
Outline Technical part TIGRE consortium Location of the telescope Technical informations Statistics Observational examples Summary
会议