Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution

MLA

Ramachandran, V., et al. Phase-Resolved Spectroscopic Analysis of the Eclipsing Black Hole X-Ray Binary M33 X-7: System Properties, Accretion, and Evolution. 2022. EBSCOhost, https://doi.org/10.1051/0004-6361/202243683.

APA

Ramachandran, V., Oskinova, L. M., Hamann, W.-R., Sander, A. A. C., Todt, H., Pauli, D., Shenar, T., Torrejón, J. M., Postnov, K. A., Blondin, J. M., Bozzo, E., Hainich, R., & Massa, D. (2022). Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution. https://doi.org/10.1051/0004-6361/202243683

Chicago

Ramachandran, V., L. M. Oskinova, W. -R. Hamann, A. A. C. Sander, H. Todt, D. Pauli, T. Shenar, et al. 2022. “Phase-Resolved Spectroscopic Analysis of the Eclipsing Black Hole X-Ray Binary M33 X-7: System Properties, Accretion, and Evolution.” doi:10.1051/0004-6361/202243683.