We also construct standard diagnostic diagrams and emission-line maps (EW(H α), /H α, //H α, /H β) and search for regions consistent with ionization by hot low-mass evolved stars (HOLMES) and shocks. Using our MUSE data, we investigate the origin of eDIG via kinematics, specifically the rotation velocity lags. To investigate the connection between in-plane star formation and eDIG, we measure the star formation rates (SFRs) and perform a photometric analysis of our narrowband H α imaging. We acquired Multi Unit Spectroscopic Explorer (MUSE) integral field spectroscopy and deep narrowband H α imaging of our sample galaxies. We investigate the origin of the extraplanar diffuse ionized gas (eDIG) and its predominant ionization mechanisms in five nearby (17–46 Mpc) low-mass (10 9–10 10 M ⊙) edge-on disk galaxies: ESO 157-49, ESO 469-15, ESO 544-27, IC 217, and IC 1553. Specim, Spectral Imaging Ltd., Elektroniikkatie 13, 90590 Oulu, FinlandĪims. Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spainĭepartment of Physics, Engineering Physics and Astrophysics, Queen’s University, Kingston, ON K7L 3N6, Canadaįinnish Centre of Astronomy with ESO (FINCA), Vesilinnantie 5, 20014 University of Turku, Finland Space Physics and Astronomy research unit, University of Oulu, 90014 Oulu, FinlandĮ-mail: of Astrophysics Research, School of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield AL10 9AB, UKĭepartamento de Astrofísica, Universidad de La Laguna, 38200 La Laguna, Tenerife, Spain Astronomical objects: linking to databases.Including author names using non-Roman alphabets.Suggested resources for more tips on language editing in the sciences Punctuation and style concerns regarding equations, figures, tables, and footnotes
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