Toward a better understanding of the IR spectral energy distributions of H II regions

Details Toward a better understanding of the IR spectral energy distributions of H II regions Toward a better understanding of the IR spectral energy distributions of H II regions

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..393..465l&link_type=abstract

The seventh astrophysical conference: Star formation, near and far. AIP Conference Proceedings, Volume 393, pp. 465-468 (1997).

Astronomy and Astrophysics

Astrophysics

Hii Regions, Emission And Reflection Nebulae, Origin, Formation, Evolution, Age, And Star Formation, Associations Of Stars In External Galaxies, Main-Sequence: Early-Type Stars

Scientific paper

Infrared spectral energy distributions (SEDs) of several isolated star-forming regions were derived from observations made by the Diffuse Infrared Background Experiment (DIRBE) on NASA's Cosmic Background Explorer (COBE). Recently obtained near-IR photometric observations of five regions will be used in conjunction with 2 μm spectroscopy to locate and classify visually obscured O and early-B stars. Our goal is to learn in some detail how the stellar population and the local interstellar environment affect the IR SED.

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