宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)
京都大学 : 東京大学 カブリ数物連携宇宙研究機構
青山学院大学
東京工業大学
宮崎大学
国立天文台
兵庫県立大学西はりま天文台
Harvard-Smithsonian Center for Astrophysics
Department of Physics, Astronomy and Geosciences, Towson University
Korea Astronomy and Space Science Institute
青山学院大学
青山学院大学
著者所属（英）
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)
Department of Astronomy, Kyoto University : Kavli Institute for the Physics and Mathematics of the universe (WPI), The University of Tokyo
Department of Physics and Mathematics, Aoyama Gakuin University
Department of Physics, Tokyo Institute of Technology
Department of Applied Physics and Electronic Engineering, Faculty of Engineering, University of Miyazaki
National Astronomical Observatory of Japan
Nishi-Harima Astronomical Observatory, Center for Astronomy, University of Hyogo
Harvard-Smithsonian Center for Astrophysics
Department of Physics, Astronomy and Geosciences, Towson University
Korea Astronomy and Space Science Institute
Department of Physics and Mathematics, Aoyama Gakuin University
Department of Physics and Mathematics, Aoyama Gakuin University
SPATIALLY RESOLVED SPECTROSCOPY OF A BALMER-DOMINATED SHOCK IN THE CYGNUS LOOP: AN EXTREMELY THIN COSMIC-RAY PRECURSOR?
