Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007astl...33...34p&link_type=abstract
Astronomy Letters, Volume 33, Issue 1, pp.34-37
Astronomy and Astrophysics
Astronomy
2
Scientific paper
We analyze the calibrations (the dependence of the spectral type of a star on its effective temperature) by comparing the calculated ionization structure of an H II region with that obtained from observations for the source Orion A in radio recombination H and He lines. The effective temperature of the star ϑ1 Ori C (the ionization source) is most likely ≈37 000 K.
Polyakov Alexander M.
Tsivilev A. P.
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