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Revista mexicana de astronomía y astrofísica
versión impresa ISSN 0185-1101
Resumen
ESPIRITU, José N.; PEIMBERT, Antonio; DELGADO-INGLADA, Gloria y RUIZ, Mara Teresa. VLT Spectroscopic analysis of HH 202. Implications on dust destruction and thermal inhomogeneities. Rev. mex. astron. astrofis [online]. 2017, vol.53, n.1, pp.95-111. ISSN 0185-1101.
We present a long-slit spectroscopic analysis of Herbig-Haro 202 and the surrounding gas of the Orion Nebula using data from the Very Large Telescope3. We determined the spatial variation of its physical conditions and chemical abundances; our results are consistent with those from previous studies albeit with improved uncertainties in some determinations. Special attention is paid to the iron (Fe) and oxygen (O) abundances, which show a peak at the brightest part of HH 202, allowing us to estimate that 57% of the dust is the destroyed; we also calculate the amount of depletion of oxygen in dust grains, which amounts to 0.126 ± 0.024 dex. Finally we show that O abundances determined from collisionally excited lines and recombination lines are irreconcilable at the center of the shock unless thermal inhomogeneities are considered.
Palabras llave : dust; extinction; Herbig-Haro objects; HII regions; ISM: abundances.