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1977•Monthly Notices of the Royal Astronomical SocietyOpen access

The effective temperature and electron pressure in the atmosphere of HD 101065

A. Przybylski

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Abstract

The effective temperature of HD 101065 derived from six-colour photometry is 6075 ± 200 K. However, because of high blanketing effect the temperature of the continuum between the absorption lines is about 460 K higher. The electron pressure in the atmosphere is not higher than in normal main sequence stars.

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The effective temperature of HD 101065 derived from six-colour photometry is 6075 ± 200 K. However, because of high blanketing effect the temperature of the continuum between the absorption lines is about 460 K higher. The electron pressure in the atmosphere is not higher than in normal main sequence stars.

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Available abstract

The effective temperature of HD 101065 derived from six-colour photometry is 6075 ± 200 K. However, because of high blanketing effect the temperature of the continuum between the absorption lines is about 460 K higher. The electron pressure in the atmosphere is not higher than in normal main sequence stars.

Key concepts: Physics, Blanketing, Effective temperature, Electron temperature, Atmosphere (unit), Stellar atmosphere, Stars, Astrophysics

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