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
Lense-Thirring Precession in the Astrophysical Context
β Scribed by Luigi Stella; Andrea Possenti
- Book ID
- 106535249
- Publisher
- Springer Netherlands
- Year
- 2009
- Tongue
- English
- Weight
- 544 KB
- Volume
- 148
- Category
- Article
- ISSN
- 0038-6308
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