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Observational Study of the Galactic Nuclear Disk using SiO Masers

Observational Study of the Galactic Nuclear Disk using SiO Masers
使用 SiO 微波激射器对银河核盘进行观测研究
批准号:
12640243
负责人:
DEGUCHI Shuji
金额:
$2.3万
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
2000
资助国家:
日本
项目状态:
已结题
起止时间:
2000 至 2002

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项目成果

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中文摘要
翻译
在2001-2003年为期三年的研究中,我们进行了以下观察。1. 使用多波束接收器对银河系中心20弧分范围内的SiO脉泽源进行浅层调查。2. 银河系核盘SiO脉泽中300个大振幅变量的研究。3. Sgr A^*和周围SiO脉泽源的VLBA观测。S. Deguchi主要关注观察1和2,以及相关的数据缩减,M. Miyoshi关注观察3。通过观测1和2,我们发现有几颗恒星具有非常高的径向速度,并且旋转速度场由两个分量组成。通过对银河系中心SiO脉泽的监测观测,我们发现与IRs10相关的脉泽在2002年5月至12月期间再次爆发。因此,我们在2003年1月再次进行了VLBI观测。这些数据目前正在由三吉先生进行处理。从2000年7月的观测中,我们得到了IRs10相对于Sgr A^*的正确运动。此外,我们还对Sgr A^*进行了高分辨率成像。根据这一分析,我们发现人马座A^*的强度和发射分布在几小时内会发生变化。因为这是由于Sgr A^*的耀斑,我们在世界上第一个发现了Sgr A^*耀斑的变化。这些新结果发表在夏威夷举行的国际研讨会上。我们仍然有几个未观测到的大振幅变量,将在今年夏天完成观测。
英文摘要
In a three-year research during 2001-2003, we performed the following observations. 1. A shallow survey of SiO maser sources in a area of 20 arcminutes toward the galactic center using a multi-beam receiver. 2. A survey of300 Large Amplitude Variables in SiO masers in the Galactic nuclear disk. 3. VLBA observations of Sgr A^* and SiO maser sources around it. S. Deguchi mainly concerned with observations 1 and 2, and associated data reductions, and M. Miyoshi concerned with the observation 3. With observations 1 and 2, we found that there are several stars with very high radial velocities, and that the rotational velocity field consists of two components. With monitoring observations of the Galactic center SiO masers, we found that the masers associated with IRs10 flared again during May - December 2002. Therefore, we made VLBI observations again in 2003 January. The data are now under processing by M. Miyoshi. From the observations made in July 2000, we obtained the proper motion of IRs10 relative to Sgr A^*. In addition, we performed the high resolution imaging of Sgr A^*. According to this analysis, it was tuend out that the intensity and emission distribution of Sgr A^* varies within a few hours. Because this is due to flares of Sgr A^*, we discovered the variation of the Sgr A^* flare first in the world. These new results were presented in the international symposium at Hawaii. We still have several Large Amplitude Variables unobserved and will finish observations this summer.
期刊论文(19)
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科研奖励(0)
会议论文
Nakashima, N., Deguchi, S.: "SiO Maser Survey of Cold IRAS Sources"Publication of Astronomical Society of Japan. 55. 229-246 (2003)
Nakashima, N., Deguchi, S.:“SiO Maser Survey of Cold IRAS Sources”日本天文学会出版物。
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通讯作者:
Deguchi et al.: "Observations of SiO Maser Sources within a Few Parsec from the Galactic Center"Publication of Astronomical Society of Japan. 54. 61-71 (2002)
Deguchi 等人:“距银河中心几秒差距内 SiO 脉泽源的观测”日本天文学会出版。
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共 16 条
    Observational Study of the SiO Maser Sources at the Galactic Center Region
    • 批准号:
      10640238
    • 项目类别:
      Grant-in-Aid for Scientific Research (C)
    • 资助金额:
      $1.92万
    • 财政年份:
      1998
    • 负责人:
      DEGUCHI Shuji
    • 依托单位:
    Research on Galactic dynamics with maser sources
    • 批准号:
      08640337
    • 项目类别:
      Grant-in-Aid for Scientific Research (C)
    • 资助金额:
      $1.41万
    • 财政年份:
      1996
    • 负责人:
      DEGUCHI Shuji
    • 依托单位:
    Observational and theoretical studies of high-velocity components of extragalactic water masers
    • 批准号:
      05640317
    • 项目类别:
      Grant-in-Aid for General Scientific Research (C)
    • 资助金额:
      $1.47万
    • 财政年份:
      1993
    • 负责人:
      DEGUCHI Shuji
    • 依托单位:
    国内基金
    海外基金
    Galaxy Analytical Modeling Evolution (GAME) and cosmological hydrodynamic simulations.
    • 批准号:
    • 项目类别:
      省市级项目
    • 资助金额:
      10.0万元
    • 批准年份:
      2025
    • 负责人:
      Antonios Katsianis
    • 依托单位: