Outburst characteristics of transient  low-mass X-ray binary 4U 1608-52

We present a detailed analysis of the long-term X-ray light curve of 4U 1608–52, focusing on fast-rising exponential-decay (FRED) outbursts, low-intensity states, and quiescent intervals. By calibrating the onset times of the outbursts, we identify three distinct classes for the FRED-type events: (i) the long-high outbursts, exceeding ~50 d in duration with peak count rates above ~40 cnt s-1; (ii) the short-medium outbursts, with durations of ~20 d and peak count rates of ~30-50 cnt s-1; and (iii) the short-low outbursts, also lasting ~20 d but reaching only ~20-30 cnt s-1 at peak. Furthermore, we examine the relation between preoutburst duration and the peak and integrated count rates of the upcoming outburst. We show that outbursts following longer quiescent periods tend to be more energetic.

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Publication Details

Journal
TURKISH JOURNAL OF PHYSICS
Published
2026-02-18
DOI
https://doi.org/10.55730/1300-0101.2801
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.00

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article

Outburst characteristics of transient  low-mass X-ray binary 4U 1608-52

Can Güngör
TURKISH JOURNAL OF PHYSICS
Astrophysical Phenomena and Observations
article

Outburst characteristics of transient  low-mass X-ray binary 4U 1608-52

Can Güngör
article en

Abstract

We present a detailed analysis of the long-term X-ray light curve of 4U 1608–52, focusing on fast-rising exponential-decay (FRED) outbursts, low-intensity states, and quiescent intervals. By calibrating the onset times of the outbursts, we identify three distinct classes for the FRED-type events: (i) the long-high outbursts, exceeding ~50 d in duration with peak count rates above ~40 cnt s-1; (ii) the short-medium outbursts, with durations of ~20 d and peak count rates of ~30-50 cnt s-1; and (iii) the short-low outbursts, also lasting ~20 d but reaching only ~20-30 cnt s-1 at peak. Furthermore, we examine the relation between preoutburst duration and the peak and integrated count rates of the upcoming outburst. We show that outbursts following longer quiescent periods tend to be more energetic.

TURKISH JOURNAL OF PHYSICSVol. 50(1)
National Aeronautics and Space Administration, Türkiye Bilimsel ve Teknolojik Araştırma Kurumu, Goddard Space Flight Center, Japan Aerospace Exploration Agency, RIKEN
Openalex Percentile: Top 46%
Astrophysical Phenomena and Observations
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