Black hole mass determination in the X-ray binary 4U 1630--47: Scaling of spectral and variability characteristics

TL;DR

This study analyzes spectral and timing data from the black hole candidate 4U 1630--47, applying scaling techniques to estimate its mass and inclination, and demonstrates characteristic spectral state transitions and correlations consistent with black hole behavior.

Contribution

It introduces a scaling method based on spectral and variability correlations to estimate black hole mass and inclination in 4U 1630--47, validated against other known black hole systems.

Findings

Black hole mass estimated at ~10 solar masses.

Spectral index saturates at high accretion rates.

Gamma correlates with QPO frequency and saturates at ~3.

Abstract

We present the results of a comprehensive investigation on the evolution of spectral and timing properties of the Galactic black hole candidate 4U 1630--47 during its spectral transitions. In particular, we show how a scaling of the correlation of the photon index of the Comptonized spectral component Gamma with low frequency of quasi-periodic oscillations (QPO), nu_L and mass accretion rate, $\dot M$ can be applied to the black hole mass and the inclination angle estimates. We analyze the transition episodes observed with the {\it Rossi} X-ray Timing Explorer (RXTE) and BeppoSAX satellites. We find that the broadband X-ray energy spectra of 4U~1630--47 during all spectral states can be modeled by a combination of a thermal component, a Comptonized component and a red-skewed iron line component. We also establish that Gamma monotonically increases during transition from the low-hard state to the high-soft state and then saturates for high mass accretion rates. The index saturation levels vary for different transition episodes. Correlations of Gamma versus nu_L also shows saturation at Gamma ~ 3. Gamma-Mdot and Gamma-nu_L correlations with their index saturation revealed in 4U~1630--47 are similar to those established in a number of other BHCs and can be considered as an observational evidence for the presence of a black hole in these sources. The scaling technique, which relies on XTE J1550--564, GRO 1655-40 and H 1743-322 as reference sources, allows us to evaluate a black hole mass in 4U~1630--47 yielding M_{BH}~10+/- 0.1 solar masses, and to constrain the inclination angle of i< 70 degrees.