Models of FeII emission in infrared and optical wavelength range

Details Models of FeII emission in infrared and optical wavelength range Models of FeII emission in infrared and optical wavelength range

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...186.2113v&link_type=abstract

American Astronomical Society, 186th AAS Meeting, #21.13; Bulletin of the American Astronomical Society, Vol. 27, p.840

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We present new calculations of the FeII emission in infrared and optical wavelength range in optically thin and optically thick cases. The calculations are based on 16-level, 35-level, 52-level, 142-level, and 920-level models; collisional excitation and radiative pumping are included. Implications of the results to models of FeII emission in the Orion Nebula and in quasars are discussed.

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