A note on the temperature of HD 101065

Details A note on the temperature of HD 101065 A note on the temperature of HD 101065

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...257l..83p&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 257, June 15, 1982, p. L83-L86.

Astronomy and Astrophysics

Astrophysics

9

Late Stars, Stellar Temperature, Abundance, F Stars, H Alpha Line, Infrared Spectra, Iron, Paschen Series, Spectral Line Width, Stellar Color, Stellar Spectra, Stellar Spectrophotometry, Ubv Spectra

Scientific paper

The claim of Kurtz and Wegner (1979) that the lines of the Paschen series have an equivalent width of up to 4 A in HD 101065 cannot be confirmed. Their strength is only about 1% of that amount. Consequently, the temperature of HD 101065 cannot be as high as 7400 K, as Kurtz and Wegner claim. Several criteria show that HD 101065 is a late F star, most likely an F8 star.

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