Štefl, S., Rivinius, T. J., & Stahl, O. (2005). FY CMa: A candidate [Phi] per-like Be+sdO binary. The nature and evolution of disks around hot stars.
Chicago Style (17th ed.) CitationŠtefl, Stanislav, Thomas J. Rivinius, and Otmar Stahl. "FY CMa: A Candidate [Phi] Per-like Be+sdO Binary." The Nature and Evolution of Disks Around Hot Stars 2005.
MLA (9th ed.) CitationŠtefl, Stanislav, et al. "FY CMa: A Candidate [Phi] Per-like Be+sdO Binary." The Nature and Evolution of Disks Around Hot Stars, 2005.
Warning: These citations may not always be 100% accurate.