e-Article
Spatially resolved properties of the ionized gas in the H ii galaxy J084220+115000.
Document Type
Article
Author
Fernández-Arenas, D; Carrasco, E; Terlevich, R; Terlevich, E; Amorín, R; Bresolin, F; Chávez, R; González-Morán, A L; Rosa-González, D; Mayya, Y D; Vega, O; Zaragoza-Cardiel, J; Méndez-Abreu, J; Izazaga-Pérez, R; Gil de Paz, A; Gallego, J; Iglesias-Páramo, J; García-Vargas, M L; Gómez-Alvarez, P; Castillo-Morales, A
Source
Subject
*IONIZED gases
*DWARF galaxies
*ELECTRON density
*GALAXIES
*SUPERGIANT stars
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Language
ISSN
0035-8711
Abstract
We present a spatially resolved spectroscopic study for the metal poor H ii galaxy J084220+115000 using MEGARA Integral Field Unit observations at the Gran Telescopio Canarias. We estimated the gas metallicity using the direct method for oxygen, nitrogen, and helium and found a mean value of 12 + log (O/H) = 8.03 ± 0.06, and integrated electron density and temperature of ∼161 cm−3 and ∼15400 K, respectively. The metallicity distribution shows a large range of Δ(O/H) = 0.72 dex between the minimum and maximum (7.69 ± 0.06 and 8.42 ± 0.05) values, unusual in a dwarf star-forming galaxy. We derived an integrated log (N/O) ratio of −1.51 ± 0.05 and found that both N/O and O/H correspond to a primary production of metals. Spatially resolved maps indicate that the gas appears to be photoionized by massive stars according to the diagnostic line ratios. Between the possible mechanisms to explain the starburst activity and the large variation of oxygen abundance in this galaxy, our data support a possible scenario where we are witnessing an ongoing interaction triggering multiple star-forming regions localized in two dominant clumps. [ABSTRACT FROM AUTHOR]