On the nature of the exciting source in G333.6-0.2

Details On the nature of the exciting source in G333.6-0.2 On the nature of the exciting source in G333.6-0.2

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.192...21l&link_type=abstract

In ESA Galactic and Extragalactic Infrared Spectroscopy p 21-22 (SEE N83-18593 08-88)

Computer Science

Hydrogen Recombinations, Infrared Spectroscopy, Molecular Clouds, Near Infrared Radiation, Stellar Spectrophotometry, Bolometers, Giant Stars, Interstellar Extinction, Ionization, Molecular Spectroscopy, Nebulae, Stellar Luminosity

Scientific paper

The measurement of hydrogen recombination lines between approximately 1.7 and 4.6 microns in G333.6 to 0.2 provides an accurate measure of the near infrared extinction and allows determination of the stellar contribution to be observed continuum. The near infrared stellar continuum is compatible with the observed bolometric luminosity and the ionization structure of the nebula only if the exciting source is a massive premansequence star (approximately 150 solar masses) or a small system of 0 type supergiants.

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