Determination of the Electron Density in the Orion Nebula with High Spectral Resolution

Details Determination of the Electron Density in the Orion Nebula with High Spectral Resolution Determination of the Electron Density in the Orion Nebula with High Spectral Resolution

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..201g&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

2

H Ii Regions, Ism: Individual (Orion Nebula), Ism: Jets And Outflows, Line: Profiles, Techniques: Spectroscopic

Scientific paper

We present the results of long-slit echelle spectroscopic observations of the density-sensitive [S II] doublet in the Orion Nebula. These form part of a large-scale program to map the entire inner Orion Nebula in three dimensions at a resolution of 2'' ×1'' ×6 km /s and in multiple optical emission lines, covering a wide range of ionization stages.

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