학술논문
Spatially-resolved properties of the ionized gas in the HII galaxy J084220+115000
Document Type
Working Paper
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.; de Paz, A. Gil; Gallego, J.; Iglesias-Páramo, J.; García-Vargas, M. L.; Gómez-Alvarez, P.; Castillo-Morales, A.; Cardiel, N.; Pascual, S.; Pérez-Calpena, A.
Source
Subject
Language
Abstract
We present a spatially resolved spectroscopic study for the metal poor HII 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\pm$0.06, and integrated electron density and temperature of $\sim161$ cm$^{-3}$ and $\sim15400$ K, respectively. The metallicity distribution shows a large range of $\Delta$(O/H) = 0.72 dex between the minimum and maximum (7.69$\pm$0.06 and 8.42$\pm$0.05) values, unusual in a dwarf star-forming galaxy. We derived an integrated $\log$(N/O) ratio of $-1.51\pm0.05$ 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.
Comment: 24 pages, 26 figures, Accepted for publication in MNRAS
Comment: 24 pages, 26 figures, Accepted for publication in MNRAS