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3D-spectroscopy of SBS star-forming galaxies
2016
Proceedings of the International Astronomical Union
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In the base of our studies of star-forming processes are the data provided by panoramic spectroscopy of galaxies composing our SBS subsample. Observations with multi-pupil spectrographs are organized in a way to obtain the spectral range centered in permitted hydrogen Hα Balmer line, by capturing at least the forbidden doublets of nitrogen [NII]6548,6583 and sulfur [SII]6716,6731. The results obtained are the spatial distributions across the targets of emission intensities and derived
doi:10.1017/s1743921316011571
fatcat:ysbe4e4iyrhjfbvj7yzyza4zru