A Robba
A transient ultraluminous X-ray source in NGC 55
Robba, A; Pinto, C; Pintore, F; Rodriguez, G; Ambrosi, E; Barra, F; Cusumano, G; D’Aì, A; Del Santo, M; Kosec, P; Marino, A; Middleton, M; Roberts, T; Salvaggio, C; Soria, R; Wolter, A; Walton, D
Authors
C Pinto
F Pintore
G Rodriguez
E Ambrosi
F Barra
G Cusumano
A D’Aì
M Del Santo
P Kosec
A Marino
M Middleton
Professor Tim Roberts t.p.roberts@durham.ac.uk
Professor
C Salvaggio
R Soria
A Wolter
D Walton
Abstract
Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 1039 erg s−1. The average number of ULXs 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 1038 erg s−1 in a 2010 XMM-Newton observation. Thanks to new and deeper observations (∼ 130 ks each), we show that the source reaches a luminosity peak >1.6 × 1039 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 ULXs. 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 ULXs.
Citation
Robba, A., Pinto, C., Pintore, F., Rodriguez, G., Ambrosi, E., Barra, F., …Walton, D. (2022). A transient ultraluminous X-ray source in NGC 55. Monthly Notices of the Royal Astronomical Society, 515(4), 4669-4674. https://doi.org/10.1093/mnras/stac2018
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 13, 2022 |
Online Publication Date | Jul 22, 2022 |
Publication Date | 2022-10 |
Deposit Date | Aug 1, 2022 |
Publicly Available Date | Aug 1, 2022 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 515 |
Issue | 4 |
Pages | 4669-4674 |
DOI | https://doi.org/10.1093/mnras/stac2018 |
Related Public URLs | https://doi.org/10.48550/arXiv.2207.09447 |
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Accepted Journal Article
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Copyright Statement
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record [Robba, A, Pinto, C, Pintore, F, Rodriguez, G, Ambrosi, E, Barra, F, Cusumano, G, D’Aì, A, Del Santo, M, Kosec, P, Marino, A, Middleton, M, Roberts, T, Salvaggio, C, Soria, R, Wolter, A & Walton, D (2022). A transient ultraluminous X-ray source in NGC 55. Monthly Notices of the Royal Astronomical Society 515(4): 4669–4674.] is available online at: https://doi.org/10.1093/mnras/stac2018
Published Journal Article
(800 Kb)
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