✦ LIBER ✦

Lithium in black hole binaries: the case of X-ray Nova Muscae 1991

✍ Scribed by E.L. Martín; J. Casares; P. Molaro; R. Rebolo; P. Charles

Book ID: 108495185
Publisher: Elsevier Science
Year: 1996
Tongue: English
Weight: 499 KB
Volume: 1
Category: Article
ISSN: 1384-1076
DOI: 10.1016/s1384-1076(96)00014-0

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Evidence for a black hole in the X-ray n

Evidence for a black hole in the X-ray nova Muscae 1991

✍ Valle, M. Della; Jarvis, B. J.; West, R. M. 📂 Article 📅 1991 🏛 Nature Publishing Group 🌐 English ⚖ 367 KB

The Masses of Black Holes in X-ray Binar

The Masses of Black Holes in X-ray Binary Systems

✍ A.M. Cherepashchuk 📂 Article 📅 1997 🏛 Springer Netherlands 🌐 English ⚖ 682 KB

The evolution of intermediate mass black

The evolution of intermediate mass black holes in X-ray binaries

✍ Simon Portegies Zwart 📂 Article 📅 2010 🏛 Elsevier Science 🌐 English ⚖ 363 KB

The remarkable stability of probable bla

The remarkable stability of probable black hole low-mass X-ray binaries in nearby galaxies

✍ J. A. Irwin 📂 Article 📅 2006 🏛 John Wiley and Sons 🌐 English ⚖ 198 KB

Bifurcation timescales in power spectra

Bifurcation timescales in power spectra of black hole binaries and ultraluminous X-ray sources

✍ TaiShan Wang; TiPei Li 📂 Article 📅 2010 🏛 Science in China Press (SCP) 🌐 English ⚖ 508 KB

The formation of high-mass black holes i

The formation of high-mass black holes in low-mass X-ray binaries

✍ G.E. Brown; C.-H. Lee; Hans A. Bethe 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 94 KB

We suggest that high-mass black holes; i.e., black holes of several solar masses, can be formed in binaries with low-mass main-sequence companions, provided that the hydrogen envelope of the massive star is removed in common envelope evolution which begins only after the massive star has finished He