Reflecting on accretion in neutron star low-mass X-ray binaries
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s10509-024-04281-y.pdf
Reference133 articles.
1. Bahramian, A., Degenaar, N.: Low-mass X-ray binaries. In: Bambi, C., Santangelo, A. (eds.) Handbook of X-ray and Gamma-Ray Astrophysics, pp. 120 (2023). https://doi.org/10.1007/978-981-16-4544-0_94-1
2. Bardeen, J.M., Press, W.H., Teukolsky, S.A.: Rotating black holes: locally nonrotating frames, energy extraction, and scalar synchrotron radiation. Astrophys. J. 178, 347–370 (1972). https://doi.org/10.1086/151796
3. Barret, D.: The broad band X-ray/hard X-ray spectra of accreting neutron stars. Adv. Space Res. 28(2–3), 307–321 (2001). https://doi.org/10.1016/S0273-1177(01)00414-8. arXiv:astro-ph/0101295 [astro-ph]
4. Barret, D., Olive, J.F., Boirin, L., et al.: Hard X-ray emission from low-mass X-ray binaries. Astrophys. J. 533(1), 329–351 (2000). https://doi.org/10.1086/308651. arXiv:astro-ph/9911042 [astro-ph]
5. Bhattacharyya, S., Strohmayer, T.E.: Evidence of a broad relativistic iron line from the neutron star low-mass X-ray binary serpens X-1. Astrophys. J. Lett. 664(2), L103–L106 (2007). https://doi.org/10.1086/520844. arXiv:0708.3648 [astro-ph]
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