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Ionization structure of the nebula NGC 6857

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Abstract

We present the results of our spectroscopic studies of the nebula NGC 6857 located in a region of current star formation. Data on the surface brightness distribution in the central region of the nebula (∼60″ × 60″) in the Hα, Hβ, [OIII], 5007 Å, [N II], 6548, 6583 Å, [S II], 6717, 6731 Å, and He I, 6678 Å lines have been obtained with an angular resolution of ∼4.″5 × 4.″5. The zones of maximum surface brightness and the region of maximum gas ionization ratio are located 12″ south of the central star, which may suggest the existence of a second gas ionization source.

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Correspondence to L. N. Kondrat’eva.

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Original Russian Text © L.M. Kondrat’eva, F.K. Rspaev, E.K. Aimuratov, 2014, published in Pis’ma v Astronomicheskiĭ Zhurnal, 2014, Vol. 40, No. 11, pp. 774–782.

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Kondrat’eva, L.N., Rspaev, F.K. & Aimuratov, E.K. Ionization structure of the nebula NGC 6857. Astron. Lett. 40, 704–712 (2014). https://doi.org/10.1134/S1063773714110024

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