supposedly constructed around 700 AD, and it is the oldest celestial map in East Asia
(Miyajima 1999).
References
Araki, T. (1925). Uber die Erklarungshypothesen der Cepheidenerscheinung. Memoirs of College
of Science, Kyoto Imperial University, Series A, 8, 75–129.
Araki, T. (1934). Zur Theorie des inneren Aufbaues der weissen Zwerge. Zeitschrift für
Astrophysik, 8, 358–369.
Araki, T. (1940). Works of late Takeda Shin-ichiro on theoretical astrophysics (荒木俊馬: 理論天
体物理学における竹田新一郎の業績). Yusei kara Kosei he (From Planets to Stars, 竹田新
一郎: 遊星から恒星へ), 245–256).
Araki, T., & Kurihara, M. (1937). Zur Konturberechnung der Emissionslinien der expandierended
Gashülle eines Sternes. Zeitschrift für Astrophysik, 13, 89–102.
Baldwin, R. B. (1949). The face of the moon. Chicago: University of Chicago Press.
Beals, C. S. (1929). On the nature of Wolf-Rayet emission. Monthly Notice of the Royal Astronomical Society, 90, 202–212.
Beals, C. S. (1934a). Spectrophotometric studies of WR stars and novae. Publication of Dominion
Astrophysical Observatory, 6, 95–145.
Beals, C. S. (1934b). P Cygni and radial ejection. Observatory, 57, 378.
Bowen, I. S. (1927). The origin of nebulium spectrum. Nature, 120, 473.
Chandrasekhar, S. (1933). The equilibrium of distorted polytropes. Monthly Notice of the Royal
Astronomical Society, 93, 539–574.
Fig. 4.27 Identification chart of Chinese constellations on astronomical map on ceilling of Kitora
Tumulus. (Miyajima 1999)
114
4 Astronomy in Early Showa. II. Kyoto 1926–1945
(Miyajima 1999).
References
Araki, T. (1925). Uber die Erklarungshypothesen der Cepheidenerscheinung. Memoirs of College
of Science, Kyoto Imperial University, Series A, 8, 75–129.
Araki, T. (1934). Zur Theorie des inneren Aufbaues der weissen Zwerge. Zeitschrift für
Astrophysik, 8, 358–369.
Araki, T. (1940). Works of late Takeda Shin-ichiro on theoretical astrophysics (荒木俊馬: 理論天
体物理学における竹田新一郎の業績). Yusei kara Kosei he (From Planets to Stars, 竹田新
一郎: 遊星から恒星へ), 245–256).
Araki, T., & Kurihara, M. (1937). Zur Konturberechnung der Emissionslinien der expandierended
Gashülle eines Sternes. Zeitschrift für Astrophysik, 13, 89–102.
Baldwin, R. B. (1949). The face of the moon. Chicago: University of Chicago Press.
Beals, C. S. (1929). On the nature of Wolf-Rayet emission. Monthly Notice of the Royal Astronomical Society, 90, 202–212.
Beals, C. S. (1934a). Spectrophotometric studies of WR stars and novae. Publication of Dominion
Astrophysical Observatory, 6, 95–145.
Beals, C. S. (1934b). P Cygni and radial ejection. Observatory, 57, 378.
Bowen, I. S. (1927). The origin of nebulium spectrum. Nature, 120, 473.
Chandrasekhar, S. (1933). The equilibrium of distorted polytropes. Monthly Notice of the Royal
Astronomical Society, 93, 539–574.
Fig. 4.27 Identification chart of Chinese constellations on astronomical map on ceilling of Kitora
Tumulus. (Miyajima 1999)
114
4 Astronomy in Early Showa. II. Kyoto 1926–1945