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  The ultraluminous X-ray Sources population of the galaxy NGC 7456

Pintore, F., Marelli, M., Salvaterra, R., Israel, G. L., Castillo, G. A. R., Esposito, P., et al. (2020). The ultraluminous X-ray Sources population of the galaxy NGC 7456. The Astrophysical Journal, 890(2): 166. doi:10.3847/1538-4357/ab6ffd.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0006-875A-D Version Permalink: http://hdl.handle.net/21.11116/0000-0006-875B-C
Genre: Journal Article

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 Creators:
Pintore, F., Author
Marelli, M., Author
Salvaterra, R., Author
Israel, G. L., Author
Castillo, G. A. Rodríguez, Author
Esposito, P., Author
Belfiore, A., Author
Luca, A. De, Author
Wolter, A., Author
Mereghetti, S., Author
Stella, L., Author
Rigoselli, M., Author
Earnshaw, H. P., Author
Pinto, C., Author
Roberts, T. P., Author
Walton, D. J., Author
Bernardini, F., Author
Haberl, F.1, Author              
Salvaggio, C., Author
Tiengo, A., Author
Zampieri, L., AuthorBachetti, M., AuthorBrightman, M., AuthorCasella, P., AuthorD'Agostino, D., AuthorDall'Osso, S., AuthorFürst, F., AuthorHarrison, F. A., AuthorMapelli, M., AuthorPapitto, A., AuthorMiddleton, M., Author more..
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Abstract: Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 1039 erg s−1. The ULX population counts several hundred objects but only a fraction are well studied. Here we present a detailed analysis of all ULXs hosted in the galaxy NGC 7456. It was observed in X-rays only once in the past (in 2005) by XMM-Newton. but the observation was short and strongly affected by high background. In 2018, we obtained a new, deeper (~90 ks) XMM-Newton observation that allowed us to perform a detailed characterization of the ULXs hosted in the galaxy. ULX-1 and ULX-2, the two brightest objects (L X ~ 6−10 × 1039 erg s−1), have spectra that can be described by a model with two thermal components, as often found in ULXs. ULX-1 also shows one order of magnitude in flux variability on short-term timescales (hundreds to thousands of kiloseconds). The other sources (ULX-3 and ULX-4) show flux changes of at least an order of magnitude, and these objects may be candidate transient ULXs, although longer X-ray monitoring or further studies are required to ascribe them to the ULX population. In addition, we found a previously undetected source that might be a new candidate ULX (labeled as ULX-5), with a luminosity of ~1039 erg s−1 and hard power-law spectral shape, whose nature is still unclear and for which a background active galactic nucleus cannot be excluded. We discuss the properties of all the ULXs in NGC 7456 within the framework of super-Eddington accretion onto stellar-mass compact objects. Although no pulsations were detected, we cannot exclude that the sources host neutron stars.

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 Dates: 2020-02-26
 Publication Status: Published online
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 Identifiers: DOI: 10.3847/1538-4357/ab6ffd
Other: LOCALID: 3237116
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Title: The Astrophysical Journal
Source Genre: Journal
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Publ. Info: Bristol; Vienna : IOP Publishing; IAEA
Pages: - Volume / Issue: 890 (2) Sequence Number: 166 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_3