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.

MLA

Reyero Serantes, S., 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 & Astrophysics / Astronomie et Astrophysique, vol. 690, Sept. 2024, pp. 1–14. EBSCOhost, https://doi.org/10.1051/0004-6361/202451324.

APA

Reyero Serantes, S., Oskinova, L., Hamann, W.-R., Gómez-González, V. M. A., Todt, H., Pauli, D., Soria, R., Gies, D. R., Torrejón, J. M., Bulik, T., Ramachandran, V., Sander, A. A. C., Bozzo, E., & 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 & Astrophysics / Astronomie et Astrophysique, 690, 1–14. https://doi.org/10.1051/0004-6361/202451324

Chicago

Reyero Serantes, S., L. Oskinova, W. -R. Hamann, V. M. A. Gómez-González, H. Todt, D. Pauli, R. Soria, et al. 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 & Astrophysics / Astronomie et Astrophysique 690 (September): 1–14. doi:10.1051/0004-6361/202451324.