Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203..417c&link_type=abstract
Astrophysical Journal, vol. 203, Jan. 15, 1976, pt. 1, p. 417-434. Research supported by the Australian Research Grants Committ
Astronomy and Astrophysics
Astrophysics
704
Bolometers, Early Stars, Radiant Flux Density, Spectral Energy Distribution, Stellar Spectrophotometry, Stellar Temperature, Astronomical Catalogs, Infrared Spectroscopy, Oao 2, Stellar Atmospheres, Stellar Luminosity, Stellar Structure, Ultraviolet Spectroscopy
Scientific paper
An empirical effective temperature for a star can be found by measuring its apparent angular diameter and absolute flux distribution. The angular diameters of 32 bright stars in the spectral range O5f to F8 have recently been measured with the stellar interferometer at Narrabri Observatory, and their absolute flux distributions have been found by combining observations of ultraviolet flux from the Orbiting Astronomical Observatory (OAO-2) with ground-based photometry. In this paper, these data have been combined to derive empirical effective temperatures and bolometric corrections for these 32 stars.
Bless Robert C.
Brown Harvey R.
Code Arthur D.
Davis Jared
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