Photoionization Modelling of HII Region with Stellar Wind Bubble Inside

Details Photoionization Modelling of HII Region with Stellar Wind Bubble Inside Photoionization Modelling of HII Region with Stellar Wind Bubble Inside

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ysc..conf...37k&link_type=abstract

YSC'16 Proceedings of Contributed Papers (eds. Choliy V. Ya., Ivashchenko G.), pp. 37-41

Computer Science

Scientific paper

The last results obtained from optimized photoionization modelling of HII region show a lack of Lyman continuum (Lyc) quanta in wavelength range 912 - 504 Å. It could be explained by the ionizing radiation penetrating the very thin and dense envelope of nebular plasma with high density. Presence of such envelope in HII region surrounding a starburst could be explained by a superwind bubble formation. For detailed analysis the multicomponent grid of photoionization models was culculated with ISM grains included. In this paper the comparative analysis of emission line spectra obtained from multicomponent modelling is presented.

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