Discovery of a transient X-ray source Suzaku J1305-4930 in NGC 4945
arXiv:2007.04465 · doi:10.1093/pasj/psaa023
Abstract
We report the serendipitous discovery of a transient X-ray source, Suzaku J13054930, 3 kpc southwest of the nucleus of the Seyfert 2 galaxy NGC 4945. Among the seven Suzaku observations of NGC 4945 from 2005 to 2011, Suzaku J13054930 was detected four times in July and August in 2010. The X-ray spectra are better approximated with a multi-color disk model than a power-law model. At the first detection on 2010 July 4--5, its X-ray luminosity was erg s and the temperature at the inner-disk radius () was keV. At the last detection with Suzaku on 2010 August 4--5, the luminosity decreased to erg s and was keV. The source was not detected on 2011 January 29, about six months after the first detection, with a luminosity upper limit of erg s. We also find an absorption feature which is similar to that reported in Cyg X-1. Assuming the standard disk, we suggest that Suzaku J13054930 consists of a black hole with a mass of 10 . The relation between the disk luminosity and is not reproduced with the standard model of a constant inner radius but is better approximated with a slim-disk model.
arXiv comment17 pages, 10 figures
References in corpus (24)
- Modelling the behaviour of accretion flows in X-ray binaries
- Cosmicflows-2: The Data
- Hard X-ray Detector (HXD) on Board Suzaku
- Monte-Carlo Simulator and Ancillary Response Generator of Suzaku XRT/XIS System for Spatially Extended Source Analysis
- Multi-Temperature Blackbody Spectrum of a Thin Accretion Disk around a Kerr Black Hole: Model Computations and Comparison with Observations
- Reproducibility of Non-X-ray Background for the X-ray Imaging Spectrometer aboard Suzaku
- In-Orbit Performance of the Hard X-ray Detector on board Suzaku
- Resolved atomic lines reveal outflows in two ultraluminous X-ray sources
- The Three Spectral Regimes Found in the Stellar Black Hole XTE J1550--564 in its High/Soft State
- The Distribution of H2O Maser Emission in the Nucleus of NGC 4945
- Corona, Jet, and Relativistic Line Models for Suzaku/RXTE/Chandra-HETG Observations of the Cygnus X-1 Hard State
- Observational Evidence for Strong Disk Comptonization in GRO J1655-40
- Chandra X-ray spectroscopy of the focused wind in the Cygnus X-1 system. I. The non-dip spectrum in the low/hard state
- XMM-Newton Observations of Ultraluminous X-Ray Sources in Nearby Galaxies
- High-resolution X-ray imaging and spectroscopy of the core of NGC 4945 with XMM-Newton and Chandra
- The X-ray reflector in NGC 4945: a time and space resolved portrait
- Simultaneous Chandra and RXTE observations of the nearby bright Seyfert 2 galaxy NGC4945
- Suzaku wide-band X-ray Spectroscopy of the Seyfert 2 AGN in NGC 4945
- Chandra X-Ray Spectroscopy of the Focused Wind in the Cygnus X-1 System. II. The Nondip Spectrum in the Low/Hard State - Modulations with Orbital Phase
- Atomic and Molecular Gas in the Starburst Galaxy NGC4945
- X-Ray Sources in the Star Forming Galaxies NGC 4194 and NGC 7541
- Super-Eddington Accretion in the Ultraluminous X-ray Source NGC1313 X-2: An Ephemeral Feast
- Discovery of a bright transient ultraluminous X-ray source Suzaku J1305-4931 in NGC 4945
- Long-term Spectral Variability of the Ultra-luminous X-ray source Holmberg IX X--1
Cited by in corpus (4)
- Extragalactic fast X-ray transient candidates discovered by Chandra (2000-2014)
- Extragalactic FXT Candidates Discovered by Chandra (2014-2022)
- A new sample of transient ultraluminous X-ray sources serendipitously discovered by Swift/XRT
- Comparing the Space Densities of Millisecond-Spin Magnetars and Fast X-Ray Transients