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The Orbit of NGC 5907 ULX-1

We report on the orbit of the binary system powering the most extreme ultraluminous X-ray pulsar known to date: NGC 5907 ULX-1 (hereafter ULX1). ULX1 has been the target of a substantial multi-instrument campaign, mainly in the X-ray band, but no clear counterparts are known in other bands. Although...

Whakaahuatanga katoa

I tiakina i:
Ngā kaituhi matua: Andrea Belfiore, Ruben Salvaterra, Lara Sidoli, Gian Luca Israel, Luigi Stella, Andrea De Luca, Sandro Mereghetti, Paolo Esposito, Fabio Pintore, Antonino D’Aì, Guillermo Rodrìguez Castillo, Dominic J. Walton, Felix Fürst, Danilo Magistrali, Anna Wolter, Matteo Imbrogno
Hōputu: Artigo
Reo:Inglês
I whakaputaina: IOP Publishing 2024-01-01
Rangatū:The Astrophysical Journal
Ngā marau:
Ultraluminous x-ray sources
Orbit determination
High mass x-ray binary stars
High time resolution astrophysics
Urunga tuihono:https://doi.org/10.3847/1538-4357/ad320a
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