On the normal energy distribution in stellar spectra: O5-O8 stars

Details On the normal energy distribution in stellar spectra: O5-O8 stars On the normal energy distribution in stellar spectra: O5-O8 stars

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42..169k&link_type=abstract

Astronomy Reports, Volume 42, Issue 2, March 1998, pp.169-173

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The spectral energy curves for a number of O4-O8 stars are analyzed using measurements taken from six sources of spectrophotometric data. Based on the normal UBV color indices for O stars, these stars are divided into three groups (O5, O6-O7, and O8), for each of which the normal energy distribution is derived and presented. Comparison of these distributions indicates clear differences between the O5 and O8 subclasses at UV wavelengths. A single normal distribution curve is, therefore, insufficient to characterize the O spectral class as a whole.

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