The [Ne III]/[Ne II] line ratio in NGC 253

Details The [Ne III]/[Ne II] line ratio in NGC 253 The [Ne III]/[Ne II] line ratio in NGC 253

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..761..429d&link_type=abstract

THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP Conference Pr

Physics

Starburst Galaxies And Infrared Excess Galaxies, Galactic Nuclei, Circumnuclear Matter, And Bulges, Origin, Formation, Evolution, Age, And Star Formation

Scientific paper

We present results of the mapping of the nucleus of the starburst galaxy NGC 253 and its immediate surroundings using the Infrared Spectrograph on board the Spitzer Space Telescope. The map is centered on the nucleus of the galaxy and spans the inner 800 × 688 pc2. We perform a brief investigation of the implications of these measurement on the properties of the star formation in this region using theories developed to explain the deficiency of massive stars in starbursts.

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