Schaefer, B. E. (2026). Orbital Period Changes of Recurrent Nova T Pyxidis Demonstrate that M_ejecta >> 11.3xM_accreted and Is Not a Type Ia Supernova Progenitor.
Chicago Style (17th ed.) CitationSchaefer, Bradley E. Orbital Period Changes of Recurrent Nova T Pyxidis Demonstrate That M_ejecta >> 11.3xM_accreted and Is Not a Type Ia Supernova Progenitor. 2026.
MLA (9th ed.) CitationSchaefer, Bradley E. Orbital Period Changes of Recurrent Nova T Pyxidis Demonstrate That M_ejecta >> 11.3xM_accreted and Is Not a Type Ia Supernova Progenitor. 2026.
Warning: These citations may not always be 100% accurate.