Cita APA (7a ed.)

Vávra, M., & Brož, M. (2026). Weak S-type asteroids compared to C-type explain the observed size distribution of the main belt.

Cita Chicago Style (17a ed.)

Vávra, Michael, y Miroslav Brož. Weak S-type Asteroids Compared to C-type Explain the Observed Size Distribution of the Main Belt. 2026.

Cita MLA (9a ed.)

Vávra, Michael, y Miroslav Brož. Weak S-type Asteroids Compared to C-type Explain the Observed Size Distribution of the Main Belt. 2026.