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H-alpha observations of Sh2-190, Sh2-222, Sh2-229, Sh2-236 HII regions

机译:SH2-190,SH2-222,SH2-229,SH2-236 HII区域的H-α观察

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摘要

Hα spectral line (6563A) profiles of four northern HII regions in the our galaxy (Sh2-190, Sh2-222, Sh2-229, Sh2-236) have been obtained using DEFPOS spectrometer, located at coude focus of 150 cm RTT150 telescope at TUBITAK National Observatory (TUG, Antalya, Turkey). Observations were carried out at nights of 2015 December 24-27 with long exposure times ranging from 900s to 3600s. The LSR velocities and the linewidths (Full Width Half Maximum: FWHM) of the Hα emission lines were found to be in the range of -45.46 kms~(-1) to +3.57 kms~(-1) and 38.50 kms~(-1) to 44.10 kms~(-1), respectively. The Sh2-229 HII region is the faintest one (211.16 R), while the Sh2-236 HII region (IC410) is brightest source (535.75 R). The LSR velocity and the line width (FWHM) results of the DEFPOS/RTT150 system were compared with the data by several authors given in literature and results of DEFPOS data were found to be in good agreement with data given in literature.
机译:使用DEFPOS光谱仪获得了我们的星系中的四个北部HII区域的Hα光谱线(6563A)曲线,位于150cm RTT150望远镜的Coude焦点位于150cm RTT150望远镜Tubitak国家天文台(拖船,安塔利亚,土耳其)。观察在2015年12月24日至27日的夜间进行,长时间曝光时间为900岁至3600s。 Hα发射线的LSR速度和线宽(全宽半最大:FWHM)为-45.46kms〜(-1)至+ 3.57公里〜(-1)和38.50公里〜( - 1)分别为44.10kms〜(-1)。 SH2-229 HII区域是最微弱的一个(211.16 r),而SH2-236 HII区域(IC410)是最亮的源(535.75 r)。 LSR速度和DEFPOS / RTT150系统的线宽(FWHM)结果与文献中的几个作者的数据进行了比较,并且发现除了除霜数据的结果与文献中给出的数据吻合良好。

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