Curé, M. (2002). Disk formation in Be-stars due to line driven stellar wind and rotation. Universidad Nacional Autónoma de México.
Chicago Style (17th ed.) CitationCuré, M. Disk Formation in Be-stars Due to Line Driven Stellar Wind and Rotation. Universidad Nacional Autónoma de México, 2002.
MLA (9th ed.) CitationCuré, M. Disk Formation in Be-stars Due to Line Driven Stellar Wind and Rotation. Universidad Nacional Autónoma de México, 2002.
Warning: These citations may not always be 100% accurate.