IR spectroscopy of Be stars
Yanina Cochetti (National University of La Plata)
Wednesday, 26th April at 3 pm.
'The IR spectra of Be stars display plenty of hydrogen recombination lines, which constitute a great tool for obtaining information on the physical and dynamic structure of different regions within the circumstellar envelope. Despite the progress that has been made in the last decades in this area, there is still a lack of synthetic spectra to compare the observational data with. Motivated by the results obtained via simultaneous J-, H-, K- and L-band spectroscopic observations of galactic Be stars, we started computing synthetic spectra with the HDUST code for different disc parameters. I will present part of those results.'