APA (7th ed.) Citation

Reyero Serantes, S., Oskinova, L., Hamann, W., Gómez-González, V. M. A., Todt, H., Pauli, D., . . . Poutanen, J. (2024). Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor. Astronomy and astrophysics, 690, . https://doi.org/10.1051/0004-6361/202451324

Chicago Style (17th ed.) Citation

Reyero Serantes, Sabela, et al. "Multi-wavelength Spectroscopic Analysis of the ULX Holmberg II X-1 and Its Nebula Suggests the Presence of a Heavy Black Hole Accreting from a B-type Donor." Astronomy and Astrophysics 690 (2024). https://doi.org/10.1051/0004-6361/202451324.

MLA (9th ed.) Citation

Reyero Serantes, Sabela, et al. "Multi-wavelength Spectroscopic Analysis of the ULX Holmberg II X-1 and Its Nebula Suggests the Presence of a Heavy Black Hole Accreting from a B-type Donor." Astronomy and Astrophysics, vol. 690, 2024, https://doi.org/10.1051/0004-6361/202451324.