2023
DOI: 10.1051/0004-6361/202347760
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NuSTAR and XMM-Newton observations of the binary 4FGL J1405.1–6119

Enzo A. Saavedra,
Federico A. Fogantini,
Gastón J. Escobar
et al.

Abstract: Context. 4FGL J1405.1−6119 is a high-mass γ-ray-emitting binary that has been studied at several wavelengths. The nature of this type of binary is still under debate, with three possible scenarios usually invoked to explain the origin of the γ-ray emission: collisions between the winds of a rapidly rotating neutron star and its companion, collisions between the winds of two massive stars, and nonthermal emission from the jet of a microquasar. Aims. We analyzed two pairs of simultaneous NuSTAR and XMM-Newton ob… Show more

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