𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The secondary stars in cataclysmic variables and low-mass X-ray binaries

✍ Scribed by D. A. Smith; V. S. Dhillon

Publisher
John Wiley and Sons
Year
1998
Tongue
English
Weight
821 KB
Volume
301
Category
Article
ISSN
0035-8711

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Superhumps in low-mass X-ray binaries
Superhumps in low-mass X-ray binaries
✍ C. A. Haswell; A. R. King; J. R. Murray; P. A. Charles πŸ“‚ Article πŸ“… 2001 πŸ› John Wiley and Sons 🌐 English βš– 118 KB
Lense-thirring precession and QPOs in lo
Lense-thirring precession and QPOs in low mass x-ray binaries
✍ Luigi Stella; Mario Vietri πŸ“‚ Article πŸ“… 1999 πŸ› Elsevier Science 🌐 English βš– 475 KB

The relativistic dragging of inertial frames around fast rotating collapsed stars is substantial and can give rise to observable effects. We apply this to the kHz quasi periodic oscillations (QPOs) sources, low mass X-ray binaries (LMXRBs) containing an accreting neutron star. Within the beat freque

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 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