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- W3036225449 abstract "Since their discovery in 1962 (Giacconi et al. 1962), accreting compact objects in the Galaxy have offered unique insights into the astrophysics of the end stages of stellar evolution and the physics of matter at extreme physical conditions. During the first three decades of exploration, new phenomena were discovered and understood, such as the periodic pulsations in the X-ray lightcurve of spinning neutron stars (Giacconi et al. 1971) and the thermonuclear flashes on neutron-star surfaces that are detected as powerful X-ray bursts (see, e.g., Grindlay et al. 1976; Chapter 3). Moreover, the masses of the compact objects were measured in a number of systems, providing the strongest evidence for the existence of black holes in the Universe (McClintock & Remillard 1986; Chapter 4)." @default.
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- W3036225449 date "2006-04-06" @default.
- W3036225449 modified "2023-10-14" @default.
- W3036225449 title "Accreting neutron stars and black holes: a decade of discoveries" @default.
- W3036225449 doi "https://doi.org/10.1017/cbo9780511536281.002" @default.
- W3036225449 hasPublicationYear "2006" @default.
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