𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries

✍ Scribed by A. V. Mescheryakov; N. I. Shakura; V. F. Suleimanov


Book ID
111437483
Publisher
Springer
Year
2011
Tongue
English
Weight
814 KB
Volume
37
Category
Article
ISSN
1063-7737

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


The formation of high-mass black holes i
✍ G.E. Brown; C.-H. Lee; Hans A. Bethe πŸ“‚ Article πŸ“… 1999 πŸ› Elsevier Science 🌐 English βš– 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