| 21. | Lambda Chamaeleontis is a K2III giant star with an effective temperature of 5000 Kelvin.
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| 22. | The minimum effective temperature depends on the various fuels, gas constituents, and catalyst geometry.
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| 23. | Nu Chamaeleontis is a G8III giant star with an effective temperature of 4800 Kelvin.
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| 24. | Sigma Ceti is an F5V Dwarf star with an effective temperature of 6600 Kelvin.
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| 25. | HD 108541 is n B8V Dwarf star with an effective temperature of 10000 Kelvin.
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| 26. | Some of its parameters were also derived, including its effective temperature and surface gravity.
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| 27. | Chi Ceti A is an F3III Giant star with an effective temperature of 6200 Kelvin.
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| 28. | The calculated effective temperature increased from 4, 500K in 1900 to 5, 000K in 1960.
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| 29. | The primary component is a outer atmosphere at an effective temperature of 14, 496 K.
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| 30. | Icy winds brought the effective temperature down to 12 degrees at Wrigley Field in Chicago.
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