1. Unveiling gas kinematics and stellar populations in H ii regions inside the low-metallicity dwarf nearby galaxy SDSSJ0859 + 3923 with MEGARA at the GTC.
- Author
-
García-Vargas, M L, Carrasco, E, Mollá, M, de Paz, A Gil, Gallego, J, Iglesias-Páramo, J, Cardiel, N, Castillo-Morales, A, Pascual, S, Gómez-Alvarez, P, and Pérez-Calpena, A
- Abstract
In this study, we present Integral Field Unit observations of the galaxy SDSSJ0859 + 3923, utilizing the MEGARA (Multi Espectrógrafo en GTC de Alta Resolución para Astronomía) instrument on the GTC (Gran Telescopio Canarias) 10.4m telescope. These observations were conducted in two distinct spectral ranges: 4332–5222 Å and 6097–7345 Å, with a high resolving power (R |$_\mathrm{FWHM}$| |$\sim 6\, 000$|), and spatial resolution of 25 pc, considering the galaxy's distance of 8.5 Mpc. Our observations have identified five H ii regions, whose precise positions were determined using data from the Wide Field Camera 3 (ultraviolet and visible) of the Hubble Space Telescope , WFC3-UVIS/ HST , archive images, where we also detected the associated blue underlying continuum linked to the ionized knots. A detailed kinematic analysis of these regions revealed low-velocity dispersion values (around 10 km s |$^{-1}$|) in four H ii regions, indicating a lack of significant turbulent events. In the fifth region, we observed a peak in velocity dispersion reaching 40 km s |$^{-1}$| , which we interpret as the result of hot star winds and/or a recent type-II supernova explosion. We have conducted a comprehensive spectral analysis of the H ii regions, obtaining emission-line fluxes that enabled us to confirm the oxygen abundance (12 + log(O/H) = 7.41 |$\pm$| 0.15) and, using popstar models, to constrain the age and mass of the ionizing young clusters. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF