Written by leading experts in the field, "Stellar Spectral Classification" is the only book to comprehensively discuss both the foundations and most up-to-date techniques of MK and other spectral classification systems. Definitive and encyclopedic, the book introduces the astrophysics of spectroscopy, reviews the entire field of stellar astronomy, and shows how the well-tested methods of spectral classification are a powerful discovery tool for graduate students and researchers working in astronomy and astrophysics. The book begins with a historical survey, followed by chapters discussing the entire range of stellar phenomena, from brown dwarfs to supernovae. The authors account for advances in the field, including the addition of the L and T dwarf classes; the revision of the carbon star, Wolf-Rayet, and white dwarf classification schemes; and the application of neural nets to spectral classification. Copious figures illustrate the morphology of stellar spectra, and the book incorporates recent discoveries from earth-based and satellite data. Many examples of spectra are given in the red, ultraviolet, and infrared regions, as well as in the traditional blue-violet optical region, all of which are useful for researchers identifying stellar and galactic spectra. This essential reference includes a glossary, handy appendixes and tables, an index, and a Web-based resource of spectra. In addition to the authors, the contributors are Adam J. Burgasser, Margaret M. Hanson, J. Davy Kirkpatrick, and Nolan R. Walborn.
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光譜學是astronomy&astrophysics中最經典也是最old school的領域,從牛頓用三棱鏡分光開始,夫琅和費使用分光儀看見瞭太陽光譜的500多條吸收綫,也是19世紀科學啓濛的重要推進力。時到今日哈佛MK分類法作為通用的恒星classifiers開始被研究者嫌棄,隨著大型巡天設備和空間探測器的發展,我們比任何時候都有更好的機會。
评分光譜學是astronomy&astrophysics中最經典也是最old school的領域,從牛頓用三棱鏡分光開始,夫琅和費使用分光儀看見瞭太陽光譜的500多條吸收綫,也是19世紀科學啓濛的重要推進力。時到今日哈佛MK分類法作為通用的恒星classifiers開始被研究者嫌棄,隨著大型巡天設備和空間探測器的發展,我們比任何時候都有更好的機會。
评分光譜學是astronomy&astrophysics中最經典也是最old school的領域,從牛頓用三棱鏡分光開始,夫琅和費使用分光儀看見瞭太陽光譜的500多條吸收綫,也是19世紀科學啓濛的重要推進力。時到今日哈佛MK分類法作為通用的恒星classifiers開始被研究者嫌棄,隨著大型巡天設備和空間探測器的發展,我們比任何時候都有更好的機會。
评分光譜學是astronomy&astrophysics中最經典也是最old school的領域,從牛頓用三棱鏡分光開始,夫琅和費使用分光儀看見瞭太陽光譜的500多條吸收綫,也是19世紀科學啓濛的重要推進力。時到今日哈佛MK分類法作為通用的恒星classifiers開始被研究者嫌棄,隨著大型巡天設備和空間探測器的發展,我們比任何時候都有更好的機會。
评分光譜學是astronomy&astrophysics中最經典也是最old school的領域,從牛頓用三棱鏡分光開始,夫琅和費使用分光儀看見瞭太陽光譜的500多條吸收綫,也是19世紀科學啓濛的重要推進力。時到今日哈佛MK分類法作為通用的恒星classifiers開始被研究者嫌棄,隨著大型巡天設備和空間探測器的發展,我們比任何時候都有更好的機會。
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