A transient ultraluminous X-ray source in NGC 55

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10(39) erg s(-1). The average number of ULX5 per galaxy is still not well-constrained, especially given the uncertainty on the fraction of ULX transients. Here, we report the identification of a new transient ULX in the galaxy NGC 55 (which we label as ULX-2), thanks to recent XMM-Newton and the Neil Gehrels Swift Observatory observations. This object was previously classified as a transient X-ray source with a luminosity around a few 10(38) erg s(-1) in a 2010 XMM-Newton observation. Thanks to new and deeper observations (similar to 130 ks each), we show that the source reaches a luminosity peak >1.6 x 10(39) erg s(-1). The X-ray spectrum of ULX-2 is much softer than in previous observations and fits in the class of soft ULXs. It can be well-described using a model with two thermal components, as often found in ULX5. The time-scales of the X-ray variability are of the order of a month and are likely driven by small changes in the accretion rate or due to super-orbital modulations, attributed to precession of the accretion disc, which is similar to other ULX5.

Automated summary

This study reports the identification of a new transient ultraluminous X-ray source (ULX-2) in the galaxy NGC 55. The source was previously classified as a transient X-ray source with a lower luminosity, but new observations show that it reaches a peak luminosity above 1.6 x 10(39) erg s(-1). The X-ray spectrum of ULX-2 is softer than in previous observations and can be described by a model with two thermal components. The variability in X-ray emission is likely driven by small changes in the accretion rate or due to super-orbital modulations.