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Understanding the Oldest White Dwarfs: Atmospheres of Cool WDs as Extreme Physics Laboratories
Solar and Stellar Astrophysics (astro-ph.SR) Materials Science (cond-mat.mtrl-sci)
2010/12/27
Reliable modeling of the atmospheres of cool white dwarfs is crucial for understanding the atmospheric evolution of these stars and for accurate white dwarfs cosmochronology. Over the last decade {\it...
WDS-A微扫测井测斜系统电路设计
微电扫描测斜 接口电路 逻辑控制 帧计数器
2009/5/19
为了完成测斜系统传感器信号调制、控制、三总线信号驱动、转换及上传数据解调电路功能,根据三总线信号特点,设计出一套数据接口、信号采集与控制电路,帧形成及字形成电路.经过室内及十余次野外油田试验,表明:接口及信号调制控制传输电路达到功能设计要求,微电扫测斜系统电子仪传输后转换精度达到4.2‰,表示每帧数据传输时间的时间字偏差不超过0.3‰,说明该短节电路设计可靠稳定,满足功能要求。
NEW ORBIT OF BINARY STAR WDS 21044S1951 = FIN 328。
REVISED ORBITS OF TWO BINARY STARS WDS 06098S2246=RST 3442 AND WDS 08285S0230=ADS 6828=A 551
BINARY STARS WDS 08285S0230=ADS 6828=A 551 WDS 06098S2246=RST 3442
2009/4/16
REVISED ORBITS OF TWO BINARY STARS WDS 06098S2246=RST 3442 AND WDS 08285S0230=ADS 6828=A 551。
DYNAMICS OF QUADRUPLE SYSTEM FINSEN 332 = ADS 11640 = HIP 92027 = WDS 18455+0530
binaries close
2009/3/11
In 1829 Struve discovered a double star denoted as STF 2375 AB
later on. Its separation was 2 . 2. It was noticed by Finsen from the Southern Observatory
(Johannesburg) in 1953 that the component...