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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

S. Reyero Serantes,L. Oskinova,W. -R. Hamann,V. M. A. Gomez-Gonzalez,H. Todt,D. Pauli,R. Soria, D. R. Gies,J. M. Torrejon,T. Bulik,V. Ramachandran,A. A. C. Sander,E. Bozzo,J. Poutanen

ASTRONOMY & ASTROPHYSICS（2024）

Cited 0|Views5
Key words
techniques: spectroscopic,stars: black holes,stars: massive,X-rays: binaries,X-rays: individuals: Ho II X-1
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