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DEFPOS and Its First Results
作者姓名:M.ahan  .Yeingil  N.Aksaker    .Kιzιolu  M.Akyιlmaz
作者单位:Department of Physics Cukurova University,01330,Adana,Turkey,Department of Physics Cukurova University,01330,Adana,Turkey,Department of Physics Cukurova University,01330,Adana,Turkey,Department of Physics Middle East Technical University,Ankara,Turkey,Department of Physics Cukurova University,01330,Adana,Turkey
摘    要:A spectrometer was built to examine the interstellar medium (ISM) using the hydrogen Balmer a line. It is called Dual Etalon Fabry-Perot Optical Spectrometer (DEFPOS). DEFPOS will be coupled to coude exit of the 150 cm telescope (RTT150) installed at TUBITAK National Observatory (TUG). DEFPOS was ready for observations about two years ago, but work was still continuing on the RTT150 coude exit alignment. So we have started observing HII regions with DEFPOS without the RTT150. We present here some characteristics of the instrument and some of the results obtained.

关 键 词:HII区域  干涉计  大气效应  星际物质  光学分光镜

DEFPOS and Its First Results
Abstract:A spectrometer was built to examine the interstellar medium (ISM) using the hydrogen Balmer a line. It is called Dual Etalon Fabry-Perot Optical Spectrometer (DEFPOS). DEFPOS will be coupled to coude exit of the 150 cm telescope (RTT150) installed at TUBITAK National Observatory (TUG). DEFPOS was ready for observations about two years ago, but work was still continuing on the RTT150 coude exit alignment. So we have started observing HII regions with DEFPOS without the RTT150. We present here some characteristics of the instrument and some of the results obtained.
Keywords:ISM: general - ISM: HII regions - instrumentation: Interferometers - techniques: interferometric - atmospheric effect
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