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Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
general
A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole
Nature, Volume 355, No. 6361, Year 1992
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Description
THE X-ray transient source GS2023 + 338 was discovered in out-burst by the Ginga satellite in 1989 (ref. 1) and has since been identified with the previously known recurrent nova V404 Cygni2. This system is recognized to be a low-mass X-ray binary3, with X-ray behaviour similar to black hole systems4, but attempts to deduce an orbital period from photometry5-9 and spectroscopy10,11 have yielded modulations with periods from 10 minutes to 6 hours. Two years after the outburst, we have used the William Herschel Telescope to find absorption features in V404 Cyg characteristic of a late G or early K star with a radial velocity curve of amplitude 211 ± 4km s-1 and period 6.473 ± 0.001 days. The deduced mass function of 6.26±0.31 M⊙ is a firm lower limit to the mass of the compact object, which for reasonable assumptions of orbital inclination and companion star mass must be a black hole with probable mass in the range 8-15.5 M⊙. We consider this the most persuasive case yet for the existence of a black hole. © 1992 Nature Publishing Group.
Authors & Co-Authors
Casares, J.
Spain, San Cristobal de la Laguna
Instituto Astrofisico de Canarias
Charles, Philip A.
United Kingdom, London
Royal Observatory, Greenwich
Naylor, Tim T.
United Kingdom, Cambridge
Institute of Astronomy
United Kingdom, Keele
Keele University
Statistics
Citations: 189
Authors: 3
Affiliations: 4
Identifiers
Doi:
10.1038/355614a0
ISSN:
00280836