Kiyonobu Date - Academia.edu (original) (raw)
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Papers by Kiyonobu Date
Bulletin d'histoire politique, 2021
Odysseus : 東京大学大学院総合文化研究科地域文化研究専攻紀要, Mar 30, 2021
Journal of Religious Studies, 2012
Journal of Religious Studies, 2015
Journal of Religious Studies, 2010
Journal of Religious Studies, 2013
Journal of Religious Studies, 2006
Journal of Religious Studies, 2011
Journal of Religious Studies, 2007
Journal of Religious Studies, 2009
Revista chilena de obstetricia y ginecología, 2017
We present a study of the central parts of the Sagittarius dwarf spheroidal galaxy (Sgr). We foun... more We present a study of the central parts of the Sagittarius dwarf spheroidal galaxy (Sgr). We found a clear overdensity of Sgr's stars around M 54 (hereafter NS). NS is well represented by a King model and it has the characteristics of a typical dwarf elliptical nucleus. Whether this means that M 54 has spiraled into the potential well of NS or that M 54 is the real nucleus and NS has formed into its potential wells, remains an open question to be addressed.
Bulletin d'histoire politique, 2021
Odysseus : 東京大学大学院総合文化研究科地域文化研究専攻紀要, Mar 30, 2021
Journal of Religious Studies, 2012
Journal of Religious Studies, 2015
Journal of Religious Studies, 2010
Journal of Religious Studies, 2013
Journal of Religious Studies, 2006
Journal of Religious Studies, 2011
Journal of Religious Studies, 2007
Journal of Religious Studies, 2009
Revista chilena de obstetricia y ginecología, 2017
We present a study of the central parts of the Sagittarius dwarf spheroidal galaxy (Sgr). We foun... more We present a study of the central parts of the Sagittarius dwarf spheroidal galaxy (Sgr). We found a clear overdensity of Sgr's stars around M 54 (hereafter NS). NS is well represented by a King model and it has the characteristics of a typical dwarf elliptical nucleus. Whether this means that M 54 has spiraled into the potential well of NS or that M 54 is the real nucleus and NS has formed into its potential wells, remains an open question to be addressed.