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出). Astronomical Herald, 52, 51–53.
Kiyonaga, K. (1979). Life and works of Professor Araki Toshima (“荒木俊馬論文集”、清永嘉
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Kogure, T. (2008). Dawn and tradition of astronomy in Kyoto (小暮智一:京都における天文学の
草創と伝統). In One-hundred years of the Astronomical Society of Japan (日本天文学会編、
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Landau, L. (1938). Origin of stellar energy. Nature, 141, 333–334.
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Astronomische Nachrichten, 191, 29–32.
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L’Astronomie, 51, 203–218.
Milne, E. A. 1930, Monthly Notice of the Royal Astronomical Society, 91, 3–55, The analysis of
stellar structure.
Miyajima, K. (1999). Ancient star map of Japan and astronomy in East Asia (京都大学人文学報、
宮島一彦: 日本の古星図と東アジアの天文学). Journal of Humanities, Kyoto University,
82, 45–56.
Miyajima, K. (2008). History of Astronomy (宮島一彦: 天文学史). In One hundred years of the
Astronomical Society of Japan (日本天文学会編、日本の天文学の百年), Hyoronsha (評論
社) (Chapter 10, pp. 153–158).
Miyamoto, K. (Ed.) (1991). Obituaries of Miyamoto Shotato, Bright Starry Night, Private Issue (宮
本周子、「星月夜」 — 宮本正太郎追禄集)、私版.
Miyamoto, S. (1938). On the Balmer emission of the planetary nebulae. Memoirs of College of
Science, Kyoto Imperial University, Ser. A, 22, 173–202.
Miyamoto, S. (1939). Cyclic equations for O III and electron temperature of gaseous nebulae.
Memoirs of College pf Science, Kyoto Imperial University, Ser. A, 22, 249–257.
Miyamoto, S. (1941). On the internal structure of neutron stars (宮本正太郎: 中性子星の内部構
造). Japanese Memoirs of Astronomy and Geophysics, 1(3), 47–54.
Miyamoto, S. (1942a). On the radiation field of hydrogen envelopes of early emission-line stars (宮
本正太郎: 特異星水素大気内の放射場について). Acta Astronomica, 1, 119–136.
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28, B. 1.
Gerasimovič, B. P. 1934, Monthly Notice of the Royal Astronomical Society, 94, 737–764,
Non-static hydrogen chromospheres and the problem of Be stars.
Hasegawa, Y. (1993). Obituary of Professor Miyamoto h長谷川靖子、宮本正太郎先生をお偲
びしてi. Accume, 5, 118–121.
Hasegawa, Y., & Sakka, K. (Eds.). (1993). Complete works of Miyamoto Shotaro, Kyoto School of
Computer Science (長谷川靖子、作花一志編: 宮本正太郎論文集, 京都コンピュータ学
院).
Hashimoto, K. (1982). A process of science revolution as seen in Chongzhen Calendar (橋本敬造:
崇禎暦書にみる科学革命の一過程、 ). Science and Skill in Asia, Dohosha, 370–380.
Kabumoto, K. (1998). The theoretical study on astrophysics by Shin-ichiro Takeda – On energy
source of stars and stellar evolution (科学史研究, 株本訓久: 竹田新一郎の理論天体物理学
研究-恒星の熱源と進化に関する研究を中心としてー). Journal of History of Science,
Japan, 37, 206–212.
Katz, J. I. (1992). Neutron stars: Physical properties and models. In S. P. Maran & C. Sagan (Eds.),
The astronomy and astrophysics encyclopedia (pp. 761–763). Cambridge: Cambridge University Press.
Kibe, N. (1959). Reminiscence of Yamamoto Issei (天文月報、木辺成麿: 山本一清先生の思い
出). Astronomical Herald, 52, 51–53.
Kiyonaga, K. (1979). Life and works of Professor Araki Toshima (“荒木俊馬論文集”、清永嘉
一: 荒木俊馬教授の生涯と業績, 京都産業大学). In Collected paper of Araki Toshima,
Kyoto Sangyo University (pp. 609–615).
Kogure, T. (2008). Dawn and tradition of astronomy in Kyoto (小暮智一:京都における天文学の
草創と伝統). In One-hundred years of the Astronomical Society of Japan (日本天文学会編、
日本の天文学の百年)、Hyoronsha (評論社) (Chapter 3, pp. 27–35).
Landau, L. (1932). On the theory of stars. Physical Journal of the Soviet Union, 1, 285.
Landau, L. (1938). Origin of stellar energy. Nature, 141, 333–334.
Lau, H. E. (1912). Über die Helligkeit der Kometen 1911 f (Quénisset) und 1911 c (Brooks).
Astronomische Nachrichten, 191, 29–32.
Lyot, B. (1937). Quelques observations de la couronne solaire et des protuberances en 1935.
L’Astronomie, 51, 203–218.
Milne, E. A. 1930, Monthly Notice of the Royal Astronomical Society, 91, 3–55, The analysis of
stellar structure.
Miyajima, K. (1999). Ancient star map of Japan and astronomy in East Asia (京都大学人文学報、
宮島一彦: 日本の古星図と東アジアの天文学). Journal of Humanities, Kyoto University,
82, 45–56.
Miyajima, K. (2008). History of Astronomy (宮島一彦: 天文学史). In One hundred years of the
Astronomical Society of Japan (日本天文学会編、日本の天文学の百年), Hyoronsha (評論
社) (Chapter 10, pp. 153–158).
Miyamoto, K. (Ed.) (1991). Obituaries of Miyamoto Shotato, Bright Starry Night, Private Issue (宮
本周子、「星月夜」 — 宮本正太郎追禄集)、私版.
Miyamoto, S. (1938). On the Balmer emission of the planetary nebulae. Memoirs of College of
Science, Kyoto Imperial University, Ser. A, 22, 173–202.
Miyamoto, S. (1939). Cyclic equations for O III and electron temperature of gaseous nebulae.
Memoirs of College pf Science, Kyoto Imperial University, Ser. A, 22, 249–257.
Miyamoto, S. (1941). On the internal structure of neutron stars (宮本正太郎: 中性子星の内部構
造). Japanese Memoirs of Astronomy and Geophysics, 1(3), 47–54.
Miyamoto, S. (1942a). On the radiation field of hydrogen envelopes of early emission-line stars (宮
本正太郎: 特異星水素大気内の放射場について). Acta Astronomica, 1, 119–136.
References
115
