Cita APA (7a ed.)

Kuvatova, D., Ishchenko, M., Berczik, P., Veles, O., Sobodar, O., & Panamarev, T. (2026). How our proto-nuclear star cluster formed and grew due to early globular cluster disruption. I. Case of low masses.

Cita Chicago Style (17a ed.)

Kuvatova, D., M. Ishchenko, P. Berczik, O. Veles, O. Sobodar, y T. Panamarev. How Our Proto-nuclear Star Cluster Formed and Grew Due to Early Globular Cluster Disruption. I. Case of Low Masses. 2026.

Cita MLA (9a ed.)

Kuvatova, D., et al. How Our Proto-nuclear Star Cluster Formed and Grew Due to Early Globular Cluster Disruption. I. Case of Low Masses. 2026.