1972
DOI: 10.1038/235037a0
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Cygnus X-1—a Spectroscopic Binary with a Heavy Companion ?

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Cited by 444 publications
(180 citation statements)
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“…A rocket borne X-ray detector, launched in 1964, discovered the persistently bright X-ray source Cygnus X-1 [35]. Its exact nature was not clear, however, until its optical identification with the O-type star HDE 226868 [36][37][38]. Based upon measurements of the optical companion's orbital parameters, mass estimates for the compact object have ranged from 8 − 16 M , with recent estimates placing the mass at approximately 10 M [9][10][11][12].…”
Section: The Identification Of Galactic Black Hole Candidates (Gbhcs)mentioning
confidence: 99%
“…A rocket borne X-ray detector, launched in 1964, discovered the persistently bright X-ray source Cygnus X-1 [35]. Its exact nature was not clear, however, until its optical identification with the O-type star HDE 226868 [36][37][38]. Based upon measurements of the optical companion's orbital parameters, mass estimates for the compact object have ranged from 8 − 16 M , with recent estimates placing the mass at approximately 10 M [9][10][11][12].…”
Section: The Identification Of Galactic Black Hole Candidates (Gbhcs)mentioning
confidence: 99%
“…An improved X-ray source location from Uhuru and an MIT rocket flight (Rappaport et al 1971) led to the discovery of a weak transient radio source by Braes and Miley (1971) from Leiden Observatory, and independently by Hjellming and Wade (1971) at the NRAO, which subsequent Uhuru analysis showed to coincide with a change in the X-ray appearance. The greatly improved source position (figure 4) finally allowed the optical identification of 'Cyg X-1 -a Spectroscopic Binary with a Heavy companion' by Webster and Murdin (1972), at the Royal Greenwich Observatory, and Bolton (1972), at the David Dunlap Observatory in Toronto. The 'heavy' companion was HDE 226868, a supergiant star at some 2 kpc distance.…”
Section: Cygnus X-1mentioning
confidence: 99%
“…In our galaxy, we are aware of twenty of these objects, located thousands of light-years away from us. One of them provided the first direct evidence for the existence of black holes: Cygnus X-1 (Bolton, 1972;Webster & Murdin, 1972).…”
Section: Monographmentioning
confidence: 99%