Physics
Scientific paper
Jun 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..152...87t&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 152, no. 1, p. 87-90
Physics
Hot Stars, Light (Visible Radiation), Spectral Energy Distribution, Standards, Stellar Spectrophotometry, Astronomical Observatories, Solar Radiation, Stellar Spectra
Scientific paper
Based on long-term observations of the absolute energy distribution in stellar spectra (starting in 1975), and from a survey of the literature, 14 stars of early spectral type (B7 III-A7 V) were selected. The constancy of their brightness is beyond any doubt now. These stars, with visual magnitudes 0.0 to 4.8, can be recommended as spectrophotometric standards for the spectral region 310 - 750 nm.
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