Output details
9 - Physics
Keele University
Early-stage young stellar objects in the Small Magellanic Cloud
Oliveira performed the data reduction of NIR photometry obtained with SOFI at ESO/NTT, 3-5micron spectroscopy obtained at VLT/ISAAC, and quality control of the database of SPITZER/IRS spectra. Oliveira performed the analysis of all data (spectral line identification, and measurements, line fitting and modelling, object classification), and wrote up the results. Oliveira performed a thorough assessment of the properties of the gas, ice and dust in a sizeable sample of young stellar objects in the Small Magellanic Cloud, and compared these properties with those of Galactic samples, in the context of understanding star formation at low metallicity.