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分子外流
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  molecular outflow
     ~(13)CO (J = 1-0) SPECTRUM IN THE REGION OF MOLECULAR OUTFLOW:W75-N
     分子外流区W75—N的~(13)CO(J=1-0)观测
短句来源
     Mapping with 12CO J=l-0 indicates that there is a high-velocity molecular outflow near the IRAS19282+1814, which is blue monopolar.
     12COJ=1-0成图观测表明在IRAS19282+1814附近存在着一个蓝向单极高速分子外流.
短句来源
     Using 4m radio telescope of Nagoya University in Japan. we observed the 13CO (J = 1-0) spectrum (110. 2011-17 GHz) in the molecular outflow region W75 - N on December 22, 1994. The integrated intensity map of 7×7 observed points (grid =2' ) was obtained.
     使用日本国名古屋大学4m射电望远镜于1994年12月22日对分子外流区W75—N的~(13)CO(J=1-0)跃迁(110GHz)进行了观测。
短句来源
     The authors conclude that these sources are those of molecular outflow.
     通过对高速气体的空间分布的观测和分析,认为这两个源为分子外流源.
短句来源
     This indicates that the noncollimation of molecular outflow in the integrated intensity map is caused by the noncollimation of the blue-shifted component .
     这说明强度分布图中的分子外流的不准直分布是由相对于峰速度的蓝移速度成分的不准直分布所引起的。
短句来源
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  molecular outflows
     These new H2O masers are associaned with CO molecular outflows[2~5] AFGL5142,HH-3,AFGL5157,NGC2023,RNO73,20126 +4104, L1251-A.
     这些新H2O脉泽是与CO分子外流源[2-5]AFGL5142,HH-3,AFOL5157,NGC2023,RNO73,20126+4104,L1251-A成协的。
短句来源
     A STUDY OF THE NONCOLLIMATION OF C~(18)O (J=1-0)MOLECULAR OUTFLOWS IN CEPHEUS E
     在Cepheus E中C~(18)O(J=1-0)分子外流的不准直分布的研究
短句来源
     H_2O 6_(16)→5_(23) MASER IN THE REGIONS OF MOLECULAR OUTFLOWS
     分子外流区的水6_(16)→5_(23)脉泽
短句来源
     SEVEN MORE RECENTLY DISCOVERED H_2O MASERS ASSOCIATED WITH MOLECULAR OUTFLOWS
     7个新近发现的与分子外流成协的H_2O脉泽
短句来源
     Using PMO 13.7m radio telescope at Qing-Hai, the surveys on H_2O 6_(16)→5_(23) line(22GHz) were made towards the 132 regions of molecular outflows in November 1993. Three new 22GHz water maser sources with flux densities of about 60Jy are detected.
     使用中国科学院紫金山天文台青海观测站的13.7米射电望远镜于1993年11月巡视了132个分子外流区的水6_(16)→5_(23)跃迁(22GHz)。
短句来源
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  “分子外流”译为未确定词的双语例句
     DISCOVERY OF NEAR INFRARED HH OBJECTS IN MOLECULAR SOURCE L1211
     分子外流源L1211中近红外HH天体的发现(英文)
短句来源
     In addition, the signal of 22GHz water maser in DR21, which could not be detected during 1987-1990, was received this time with the flux density of around 100Jy.
     发现了3个流量在60Jy左右的新的水22GHz脉泽源,并重新观测到在1987-1990年间未能测到的DR21分子外流区的水22GHz脉泽。
短句来源
     Some young outslow sources with low and high mass were observed at the wavelength of800μm, the spectral line of COJ=3-2. Results of the scan observations of AFGL 4O29 andLl582B are given.
     本文对一批包括高、低质量年轻星体的分子外流源进行了800pm、COJ=3-2谱线的观测,同时给出了AFGL4029和L1582B两块云的扫描观测的初步结果。
短句来源
     The “Hubble” Law of the Velocity Field for Highly Collimated Bipolar Outflows
     高准直双极分子外流速度的“哈勃”律
短句来源
     To search for high-velocity molecular emission toward massive star formation regions, and To study the connections between H2O masers, IRAS objects and outflow properties, we carried out a CO observation for a H2O maser sample. We found that most of the objects have excess high velocity emission produced by outflows;
     通过在大质量恒星形成区搜寻高速分子辐射,并且研究它们与星际H_2O脉泽源和所联系的红外源之间的关系,我们发现绝大多数源都存在着气体的高速运动并且它们是由分子外流产生的;
短句来源
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  molecular outflow
12CO J=2-1 maps of L379 IRS1 show a molecular outflow seen almost end-on while C18O J=2-1 emission covers a smaller central region, tracing virially bound material deeper within the cloud.
      
We present new images of the well-known molecular outflow and Herbig-Haro complex L 1551-IRS 5.
      
In addition to a central accretion-ejection engine driving the jet, the molecular outflow is powered by the infalling matter and follows a circulation pattern around the central object without necessarily being entrained by the jet.
      
We will try to clarify the relation between the fast jet and its surrounding molecular outflow, which does not primarily rely on entrainment (prompt or turbulent) in the model.
      
Hence, there is no need to transfer a large momentum from the jet to the molecular outflow through the entrainment processes.
      
更多          
  molecular outflows
The H2O maser was discovered in May 1992 (Pashchenko 1992) during a survey of IRAS sources associated with dense cold clouds with bipolar molecular outflows.
      
High-velocity molecular outflows hear massive young stellar objects
      
By mapping the12COJ = 1-0 lines in IRAS 05391-0217, 06114 + 1745 and 06291 + 0421, three new high-velocity bipolar molecular outflows are found.
      
Bipolar molecular outflows are a ubiquitous phenomenon in the process of star formation.
      
All these areas are important for developing a plausible scenario for the formation and evolution of the bipolar molecular outflows.
      
更多          


Using PMO 13.7m radio telescope at Qing-Hai, the surveys on H_2O 6_(16)→5_(23) line(22GHz) were made towards the 132 regions of molecular outflows in November 1993. Three new 22GHz water maser sources with flux densities of about 60Jy are detected. In addition, the signal of 22GHz water maser in DR21, which could not be detected during 1987-1990, was received this time with the flux density of around 100Jy. Based on our observation, the properties of some well known strong 22GHz H_2O maser sources, i.e., Orion-KL,...

Using PMO 13.7m radio telescope at Qing-Hai, the surveys on H_2O 6_(16)→5_(23) line(22GHz) were made towards the 132 regions of molecular outflows in November 1993. Three new 22GHz water maser sources with flux densities of about 60Jy are detected. In addition, the signal of 22GHz water maser in DR21, which could not be detected during 1987-1990, was received this time with the flux density of around 100Jy. Based on our observation, the properties of some well known strong 22GHz H_2O maser sources, i.e., Orion-KL, W49, Cep-A, are discussed.

使用中国科学院紫金山天文台青海观测站的13.7米射电望远镜于1993年11月巡视了132个分子外流区的水6_(16)→5_(23)跃迁(22GHz)。发现了3个流量在60Jy左右的新的水22GHz脉泽源,并重新观测到在1987-1990年间未能测到的DR21分子外流区的水22GHz脉泽。在本次观测的基础上对Orion-KL,W49,Cep-A等著名强源的某些特征进行了讨论。

Following the ten new H2O masers detected in star-forming regions[1] published,seven more Galactic interstellar H2O masers with their related parameters and spectra are briefly given in this paper.These new H2O masers are associaned with CO molecular outflows[2~5] AFGL5142,HH-3,AFGL5157,NGC2023,RNO73,20126 +4104, L1251-A.Their mean difference in position betwcen these new masers and the corresponding central IRAS point sources of outflows is|△α|= 24".8,|△δ|=27".

本文发表继探测到恒星形成区的10个新H2O脉泽[1]后,再发现和证认的7个银河系星际H2O脉泽及其有关参量和谱线图。这些新H2O脉泽是与CO分子外流源[2-5]AFGL5142,HH-3,AFOL5157,NGC2023,RNO73,20126+4104,L1251-A成协的。它们与相应的外向流的中心IRAS点源间的平均位置差为|△α|=24''.8,|△δ|=27''。

Some young outslow sources with low and high mass were observed at the wavelength of800μm, the spectral line of COJ=3-2. Results of the scan observations of AFGL 4O29 andLl582B are given.

本文对一批包括高、低质量年轻星体的分子外流源进行了800pm、COJ=3-2谱线的观测,同时给出了AFGL4029和L1582B两块云的扫描观测的初步结果。

 
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