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/*
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* Copyright (C) 2020 Christopher J. Howard |
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* |
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* This file is part of Antkeeper source code. |
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* |
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* Antkeeper source code is free software: you can redistribute it and/or modify |
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* it under the terms of the GNU General Public License as published by |
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* the Free Software Foundation, either version 3 of the License, or |
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* (at your option) any later version. |
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* |
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* Antkeeper source code is distributed in the hope that it will be useful, |
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* but WITHOUT ANY WARRANTY; without even the implied warranty of |
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* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the |
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* GNU General Public License for more details. |
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* |
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* You should have received a copy of the GNU General Public License |
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* along with Antkeeper source code. If not, see <http://www.gnu.org/licenses/>.
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*/ |
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#ifndef ANTKEEPER_COLOR_INDEX_HPP
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#define ANTKEEPER_COLOR_INDEX_HPP
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namespace ast |
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{ |
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/**
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* Approximates the temperature of a star, given its B-V index. |
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* |
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* @see Ballesteros, F. J. (2012). "New insights into black bodies". EPL 97 (2012) 34008. |
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* |
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* @param bv B-V index. |
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* @return Temperature, in Kelvin. |
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*/ |
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double bv_to_k(double bv); |
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} // namespace ast
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#endif // ANTKEEPER_COLOR_INDEX_HPP
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