Leonid S. Pilyugin

TL;DR: In this paper, a re-analysis of spectroscopic data for 23 H-II regions in 12 blue, metal-poor, low surface brightness galaxies (LSBGs), taking advantage of recent developments in calibrating strong-line methods.

TL;DR: In this paper, the authors analyzed the distribution of the gas velocity dispersion σ across the images of 1146 MaNGA galaxies and found that there are two types of distributions of the dispersion across images of galaxies: (i) the distributions of 909 galaxies show a radial symmetry with or without the σ enhancement at the center (R distribution) and (ii) distributions with a band of enhanced σ along the minor axis in images of 159 galaxies with or with the ε enhancing at the centre (B distribution).

TL;DR: In this paper, three sets of strong lines are considered, namely, A (R PsyNet 3, R PsyNet 2, NSourceFile 2, S PsyNet 2 lines), B (RSourceFile 3, N PsyNet 2 and S PsyNet 3 lines), and C (R� 2 and N� 2 lines).

TL;DR: In this article, an analysis of the optical properties of three Ultra Luminous X-ray (ULX) sources identified in NGC 925 is presented, while the spaxel associated with ULX-2 had a low S/N, which prevented its analysis.