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Spectral observations of galaxies with UV excess

机译:紫外线过多的星系的光谱观察

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Spectral observations of 19 galaxies with UV-excesses from Kazarian's list are reported. The spectra were obtained with the 2.6-m telescope at the Byurakan Observatory using the SCORPIO spectral camera. A grism was used to obtain spectra in the wavelength interval lambda lambda 7420-3920 angstrom. 43 spectra in which emission lines are mainly observed were obtained from the 19 galaxies, except for the spectra of Kaz 21, Kaz 178, Kaz 183, and Kaz 184. The spectra of Kaz 17, Kaz 151, Kaz 153, and Kaz 357 have type Sy2 galactic features. In the spectra of the galaxies Kaz 17, Kaz 151, and Kaz 153, absorption lines are observed along with high excitation emission lines such as HeI lambda 5876 angstrom and HeII lambda 4686 angstrom. No lines were observed within the interval lambda lambda 7420-3920 angstrom in the spectra of the galaxies Kaz 183 and Kaz 184.
机译:报告了19个星系的光谱观察结果,这些星系来自Kazarian列表。光谱是使用SCORPIO光谱相机在比拉坎观象台的2.6米望远镜获得的。使用格里斯(gris)获得波长间隔为λ7420-3920埃的光谱。除了Kaz 21,Kaz 178,Kaz 183和Kaz 184的光谱外,从19个星系中获得了43个主要观察到发射线的光谱。Kaz17,Kaz 151,Kaz 153和Kaz 357的光谱具有类型Sy2银河特征。在星系Kaz 17,Kaz 151和Kaz 153的光谱中,观察到吸收线以及高激发发射线,例如HeIλ5876埃和HeIIλ4686埃。在星系Kaz 183和Kaz 184的光谱中,在λλ7420-3920埃间隔内未观察到任何线。

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