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A continuous Flaring- to Normal-branch transition in Sco X-1

Piergiorgio Casella·Tomaso Belloni·Luigi Stella
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Abstract

We report the first resolved rapid transition from a Flaring Branch Oscillation to a Normal Branch Oscillation in the RXTE data of the Z source Sco X-1. The transition took place on a time scale of ~100 seconds and was clearly associated to the Normal Branch-Flaring Branch vertex in the color-color diagram. We discuss the results in the context of the possible association of the Normal Branch Oscillation with other oscillations known both in Neutron-Star and Black-Hole systems, concentrating on the similarities with the narrow 4-6 Hz oscillations observed at high flux in Black-Hole Candidates.

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Piergiorgio Casella, Tomaso Belloni, Luigi Stella. 2005-06-21. A continuous Flaring- to Normal-branch transition in Sco X-1. https://doi.org/10.1051/0004-6361%3A20052912

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