๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Superhumps in low-mass X-ray binaries

โœ Scribed by C. A. Haswell; A. R. King; J. R. Murray; P. A. Charles

Publisher
John Wiley and Sons
Year
2001
Tongue
English
Weight
118 KB
Volume
321
Category
Article
ISSN
0035-8711

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

X-ray irradiation in low-mass binary sys
X-ray irradiation in low-mass binary systems
โœ Guillaume Dubus; Jean-Pierre Lasota; Jean-Marie Hameury; Phil Charles ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 949 KB
Lense-thirring precession and QPOs in lo
Lense-thirring precession and QPOs in low mass x-ray binaries
โœ Luigi Stella; Mario Vietri ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 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
โœ G.E. Brown; C.-H. Lee; Hans A. Bethe ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 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