Discovery of a transient X-ray source Suzaku J1305−4930 in NGC 4945

• Published in: Publications of the Astronomical Society of Japan 2020-06, Vol.72 (3)
• Main Authors: Ide, Shuntaro, Hayashida, Kiyoshi, Noda, Hirofumi, Kurubi, Hiroyuki, Yoneyama, Tomokage, Matsumoto, Hironori
• Format: Article
• Language: English
• ISSN: 0004-6264; 2053-051X
• DOI: 10.1093/pasj/psaa023

Abstract We report the serendipitous discovery of a transient X-ray source, Suzaku J1305−4930, ∼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 J1305−4930 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 $(8.9^{+0.2}_{-0.4}) \times 10^{38}\:$erg s−1 and the temperature at the inner-disk radius (kTin) was 1.12 ± 0.04 keV. At the last detection with Suzaku on 2010 August 4–5, the luminosity decreased to $(2.2^{+0.3}_{-0.8}) \times 10^{38}\:$erg s−1 and kTin was 0.62 ± 0.07 keV. The source was not detected on 2011 January 29, about six months after the first detection, with a luminosity upper limit of 2.4 × 1038 erg s−1. We also find an absorption feature which is similar to that reported in Cyg X-1. Assuming the standard disk, we suggest that Suzaku J1305−4930 consists of a black hole with a mass of ∼10 $M_\odot$. The relation between the disk luminosity and kTin is not reproduced with the standard model of a constant inner radius but is better approximated with a slim-disk model.