Abstract
Observations with the 6-m telescope of the Special Astrophysical Observatory obtained with the MPFS panoramic spectrograph and a slit spectrograph with the SCORPIO focal reducer are used to analyze the emission spectrum of the ionized gas in a star-forming region in the BCD galaxy VII Zw 403. We present images of the galaxy’s central region in Hα, Hβ, [SII], and [OIII], together with maps of the relative [OIII]/Hβ and [SII]/Hα intensities. We have determined the parameters of the gas in bright ionized supershells, and estimated the relative abundances of oxygen, nitrogen, and sulfur; a low relative N/O abundance was detected.
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Original Russian Text © V.P. Arkhipova, T.A. Lozinskaya, A.V. Moiseev, O.V. Egorov, 2007, published in Astronomicheskiĭ Zhurnal, 2007, Vol. 84, No. 11, pp. 963–974.
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Arkhipova, V.P., Lozinskaya, T.A., Moiseev, A.V. et al. The gas emission spectrum in a star-forming region in the BCD galaxy VII Zw 403 (UGC 6456). Astron. Rep. 51, 871–881 (2007). https://doi.org/10.1134/S1063772907110017
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DOI: https://doi.org/10.1134/S1063772907110017