Anomalous nature of outbursts of the black hole candidate 4U 1630-472
Kaushik Chatterjee, Dipak Debnath, Riya Bhowmick, Sujoy Kumar Nath,, Debjit Chatterjee

TL;DR
This study analyzes 13 outbursts of the black hole candidate 4U 1630-472 over two decades, revealing two distinct outburst types with different durations and recurrence patterns, suggesting the presence of two companion binaries influencing the outbursts.
Contribution
It identifies and characterizes two distinct outburst types in 4U 1630-472 and explores their evolution and possible binary companions, which is a novel insight into this source's behavior.
Findings
Normal outbursts recur approximately every 500 days.
Super outbursts last 1.5-2.5 years and include multiple normal outbursts.
A linear relation exists between quiescent and outbursting periods.
Abstract
The Galactic black hole candidate (BHC) 4U~1630-472 has gone through several outbursts (13 to be particular) in the last two and a half decades starting from the RXTE era till date. Like the outbursts of other transient BHCs, the outbursts of this source show variations in duration, peak numbers, highest peak flux, etc. However, unlike any other soft X-ray transients, this source showed outbursts of two types, such as normal and super. The normal outbursts of duration ~days are observed quasi periodically at an average recurrence/quiescence period of ~days. The super outbursts of duration ~years contain one or more normal outbursts other than one mega outburst. We make an effort to separate flux contribution of the normal and the mega outbursts from the super outbursts, and tried to understand the nature of evolution of both types (normal and mega)…
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