Fe II in the Orion Nebula: Spectroscopic Observations and Theoretical Models

Details Fe II in the Orion Nebula: Spectroscopic Observations and Theoretical Models Fe II in the Orion Nebula: Spectroscopic Observations and Theoretical Models

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12...42v&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

Galaxies: Evolution, Hydrodynamics, Ism: Structure, Stars: Formation, Supernova Remnants

Scientific paper

To create a complete numerical model of the Fe II emission we use
spectroscopic observations of the Orion Nebula obtained from the Cerro
Tololo Inter-American Observatory. We have identified 40 [Fe II] lines
in the spectrum, allowing extensive comparisons between theory and
observations.

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