脉泽

  • 网络MASER;Mega-maser
脉泽脉泽
  1. OH17.7-20的拱星OH脉泽辐射的观测

    The observation of circumstellar Oh maser radiation of Oh 17.7-2.0

  2. 星际水脉泽源中高速气体的CO巡测

    A CO Survey for High Velocity Gas in Interstellar H 2O Maser Sources

  3. 与HⅡ区成协的星际脉泽激发机制

    The excitation mechanism of interstellar masers associated with H ⅱ regions

  4. 恒星形成区H2O对脉泽的观测与研究

    Observational study of h_2o maser in the star formation region

  5. 星际HⅡ/H2O脉泽的一种激发机制

    An excitation mechanism of interstellar h ⅱ / h_2o Masers

  6. 7个新近发现的与分子外流成协的H2O脉泽

    Seven more recently discovered h_2o masers associated with molecular outflows

  7. 银河系恒星形成区的OH、H2O脉泽

    The OH and H2O Masers in the Star Forming Regions of the Galaxy

  8. 研究了这19个伴有OH1720MHz脉泽发射的混合形态超新星遗迹的X射线特征。

    The X-ray characteristics have been studied .

  9. 星际H_2O脉泽的观测与研究

    Observation Studies for H_2O masers in Star Fomation Regions

  10. 一旦分子数密度达10~7cm~(-3)量级,OH脉泽便将熄灭。

    When the molecular density is over 107 cm-3 , the OH maser will be quenched .

  11. 新的H2O脉泽源的发现与证认

    Discovery and identification of new h_2o maser sources

  12. 氢脉泽振荡参数q的实验估算及氢脉泽诊断技术

    Experimental Estimation of Hydrogen Maser 's Oscillation Parameter q and Diagnostic Technique of Hydrogen Maser

  13. 本文介绍一种实验估算氢脉泽振荡参数q的测量方法。

    This paper describes a measurement method for experimental estimating oscillation parameter q of hydrogen maser .

  14. 新近发现的H2O6(16)-5(23)脉泽速度时变的研究

    A study of time variation in LSR velocities of recently discovered h_2o6_ ( 16 ) - 5_ ( 23 ) Masers

  15. 本文评述了天体H2O脉泽的时变。

    The time variations of both interstellar H2O maser and stellar H2O maser are reviewed in this paper .

  16. 用VLBI测定H2O脉泽源的距离

    Distance Determination of H2O Maser Sources with VLBI

  17. 所有超脉泽星系显示出核的活动,显然,脉泽是由核活动所产生的射电和X射线光子或激波来抽运的。

    The AGN apparently produces the seed radio photons and the X-ray photons or shock waves need to pump the maser material .

  18. SiO脉泽星的近红外测光与分析

    Near-infrared Photometry and Analysis of SiO Maser Stars of Different Types

  19. 天体SiO脉泽谱线的观测和研究

    The Observation and Study on the Spectra of Celestial SiO Maser

  20. 利用上述模型,还讨论了H2O脉泽及其他分子吸收线和发射线的发生区域。

    According to this model the positions of H2O maser , and other molecular absorption and emission line sources are discussed .

  21. 猎户座中SiO脉泽分布的新模型

    A New Model of the SiO Maser Distribution in Orion

  22. AGB后星OH17.7-2.0附近一个新的弱OH脉泽源

    A New Weak OH Maser Source Near the Post AGB Star OH 17.7 2.0

  23. 小型TE(111)无泡隔膜腔氢脉泽的实验研究

    An Experimental Study for the Compact Hydrogen Maser with a TE_ ( 111 ) Septum Cavity

  24. 在Orion-KL中的OH脉泽的外流模型:多重分离的旋转膨胀环

    The Out-Flow Model of OH Maser in Orion-KL : Multi-Distinct Rotating and Expanding Rings

  25. 对河外星系OH超脉泽的观测和研究,是探测和研究其所成协的活动星系核、星暴星系的中央源和拱核盘的有效工具。

    The observations and studies of the OH megamasers associated with AGN and starburst galaxies are the very efficient tools to investigate characteristics of their central sources an .

  26. 空间VLBI的天体脉泽观测研究

    Future Observations of Cosmic Masers Using Space VLBI

  27. 一种用来装备中国VLBI网络的新型氢脉泽标准已在上海天艺台研制成功。

    A new hydrogen maser for VLBI-network in China has been developed at Shanghai Observatory .

  28. 本文评述了1968年发现天体H2O分子谱线以来其观测和研究的进展。内容包括(1)天体H2O脉泽和正常H2O分子的观测特征;

    The progress and current situation of observations and studies about the spectra of celestial H2O molecule since it was discovered in 1968 are reviewed in this paper .

  29. 不对称的53.3微米吸收线轮廓特征有可能成为帮助我们从观测上对OH脉泽的辐射抽运机制加以鉴别的有力工具。

    The asymmetrical 53.3 μ m absorption line profile could become a powerful tool to assist us to observationally discriminate the radiative pumping mechanism from other pumping mechanisms in the OH masers .

  30. SiO脉泽速度频谱的一种分析模型&恒星脉动对恒星包层速度结构的影响

    An Analytical Model for the Velocity Spectra of SiO Maser & the Effect of Stellar Pulsation on the Velocity Structure in Stellar Envelope