Relativistic motion in a nearby bright X-ray source

The recent discovery of radio components apparently moving away from a Galactic source of transient x-ray emission faster than the speed of light has identified a low-energy Galactic counterpart to quasars. High-resolution radio observations of a second Galactic superluminal radio source GRO J1655-4...

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Veröffentlicht in:Nature (London) 1995-03, Vol.374 (6518), p.141-143
Hauptverfasser: Tingay, S. J, Jauncey, D. L, Preston, R. A, Reynolds, J. E, Meier, D. L, Murphy, D. W, Tzioumis, A. K, McKay, D. J, Kesteven, M. J, Lovell, J. E. J, Campbell-Wilson, D, Elllngsen, S. P, Gough, R, Hunstead, R. W, Jonos, D. L, McCulloch, P. M, Migenes, V, Quick, J, Sinclair, M. W, Smits, D
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Sprache:eng
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Zusammenfassung:The recent discovery of radio components apparently moving away from a Galactic source of transient x-ray emission faster than the speed of light has identified a low-energy Galactic counterpart to quasars. High-resolution radio observations of a second Galactic superluminal radio source GRO J1655-40 are examined.
ISSN:0028-0836
1476-4687
DOI:10.1038/374141a0