Emission line analysis of two giant HII regions in M33

Details Emission line analysis of two giant HII regions in M33 Emission line analysis of two giant HII regions in M33

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..419j&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

I will present the results of the study of these two objects, based on observations made by E. Perez, R Gonzalez-Delgado and J Vilchez (IAA, Granada). These long-slit, high signal-to-noise spectra, completed by archived data from HST, IUE and ISO and ground-based images, will alow to achieve an accurate modelization of the nebulae. Their ionising sources are modelled with Starburst99; then, Stasińska's code PHOTO is to be used to understand the ionization conditions of the two nebulae.

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