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- W2100342129 abstract "Les raies sont similaires pour les deux sources et representent une raie d'emission unique a environ 6,7 keV avec une largeur intrinseque inferieure a 1,7 keV. Elles sont principalement dues a des ions du type helium (Fe XXV). Les largeurs equivalentes de la raie sont dans le domaine 30-100 eV pour Sco X-1 et 30-120 eV pour 4U 1608-52" @default.
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- W2100342129 date "1984-01-01" @default.
- W2100342129 modified "2023-09-23" @default.
- W2100342129 title "Detection of iron K-emission lines from two low-mass binary X-ray sources - Scorpius X-1 and 4U 1608-52" @default.
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