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We present a comparison of archival Spitzer spectra of the strongly variable T Tauri EX Lupi, observed before and during its 2008 outburst. We analyze the mid-infrared emission from gas-phase molecules thought to originate in a circurnstellar disk. In quiescence the emission shows a forest of H20 lines, highly excited OH lines, and the Q branches of the organics C2H2, HCN, and CO2, similar to the emission observed toward several T Tauri systems. The outburst emission shows instead remarkable changes: H20 and OH line fluxes increase, new OH, H2, and H I transitions are detected, and organics are no longer seen. We adopt a simple model of a single-temperature slab of gas in local thermal equilibrium, a common approach for molecular analyses of Spitzer spectra, and derive the excitation temperature, column density, and emitting area of H20 and OH. We show how model results strongly depend on the selection of emission lines fitted and how this is likely to be attributed to a combination of non-thermal excitation and multiple emission components. Using H20 lines that can be approximated as thermalized to a single temperature, our results are consistent with a column density decrease in outburst while the emitting area of warm gas increases. A rotation diagram analysis suggests that the OH emission can be explained with two temperature components, which remarkably increase in column density in outburst. The relative change of H20 and OH emission suggests a key role for UV radiation in the disk surface chemistry. [ABSTRACT FROM AUTHOR]

A correction to the article "Ex Lupi from quiescence to outburst: Exploring the LTE approach in modeling blended H2O and OH mid-infrared emission," by A. Banzatti, M.R. Meyer, S. Bruderer, V. Geers. I. Pascucci, F. Lahuis, A. Juhaász, T. Henning and P. ábrahám.