Discovery of a bright transient ultraluminous X-ray source, Suzaku J1305-4931 in NGC 4945

Naoki Isobe, Aya Kubota, Kazuo Makishima, Poshak Gandhi, Richard E. Griffiths, Gulab C. Dewangan, Takeshi Itoh, Tsunefumi Mizuno

Research output: Contribution to journalArticlepeer-review

16 Citations (Scopus)


An X-ray source, Suzaku J1305-4931, was discovered in the south-west arm of a nearby Seyfert II galaxy, NGC 4945, at 0.5-10 keV flux of 2.2 × 10 -12 erg Cm-2 s-1 during a Suzaku observation conducted on 2006 January 15-17. It was undetectable in a shorter observation on 2005 August 22-23, with an upper limit of 1.7 × 10-14 erg cm-2 s-1. At a distance of 3.7 Mpc, the bolometric luminosity of the source became Lbol = 4.4 × 1039 α erg s-1, where α = (cos 60°/cos i) and i is the disk inclination. The time-averaged X-ray spectrum of the source is described by a multi-color disk model, with an innermost disk temperature of Tin = 1 .69-0.05+0.06 keV. It varied by a factor of 2 in intensity, following a clear correlation of Lbol ∝ T in4. The innermost disk radius is inferred to stay constant at Rin = 79-3.9+4.0α1/2 km, suggesting the presence of a standard accretion disk. Relating Rin with the last stable orbit around a non-rotating black hole yields a rather low black-hole mass, ∼ 9α1/2 solar masses, which would imply that the source is shining at a considerable super-Eddington luminosity. These results can be better interpreted by invoking sub-Eddington emission from a rapidly spinning black hole with 20-130 solar masses.

Original languageEnglish
Pages (from-to)S241-S250
JournalPublications of the Astronomical Society of Japan
Issue numberSPEC. ISS. 1
Publication statusPublished - 2008


  • Accretion, accretion disks
  • Black hole physics
  • Galaxies: individual (NGC 4945)
  • X-rays: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'Discovery of a bright transient ultraluminous X-ray source, Suzaku J1305-4931 in NGC 4945'. Together they form a unique fingerprint.

Cite this