On the hydrogen recombination radio lines in H II regions of high emission measure

Astronomy and Astrophysics – Astronomy

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Emission Spectra, H Ii Regions, Hydrogen Recombinations, Interstellar Gas, Radio Astronomy, Energy Levels, Quantum Numbers, Stark Effect

Scientific paper

The recombination line enhancement of radio lines in H II regions with high emission measure (up to about 10,000,000 pc per 0.000001 cm) is calculated, using general expressions for recombination intensities and an allowance for Stark line-broadening effects. It is found that there exists a range of values of the principal quantum number n for which strongly enhanced recombination lines of hydrogen might be detectable. Numerical values for the enhancement and the characteristic line/continuum ratio are given in the form of curves representing the functions of n for several levels of electron density.

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