A 12.6-ms pulsar in Cygnus X-3

The X-ray binary Cygnus X-3 has long been suspected of containing a fast, young pulsar, but previous observations at various wavelengths have failed to provide any evidence of a signal with a periodicity of less than 4.8 h (the well-known periodicity in the X-ray and infrared wavebands which is ascr...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Nature (London) 1985-12, Vol.318 (6047), p.642-644
Hauptverfasser: Dipper, N. A, Dowthwaite, J. C, Walmsley, M, Chadwick, P. M, Kirkman, I. W, Turver, K. E, McComb, T. J. L, Harrison, A. B, Orford, K. J, Macrae, J. H, Gibson, A. I, Lotts, A. P
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!