Deep X-Ray and Radio Observations of the First Outburst of the Young Magnetar Swift J1818.0−1607

Swift J1818.0−1607 is a radio-loud magnetar with a spin period of 1.36 s and a dipolar magnetic field strength of B ∼ 3 × 10 ^14 G, which is very young compared to the Galactic pulsar population. We report here on the long-term X-ray monitoring campaign of this young magnetar using XMM-Newton, NuSTA...

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Bibliografske podrobnosti

Principais autores:	A. Y. Ibrahim, A. Borghese, N. Rea, F. Coti Zelati, E. Parent, T. D. Russell, S. Ascenzi, R. Sathyaprakash, D. Götz, S. Mereghetti, M. Topinka, M. Rigoselli, V. Savchenko, S. Campana, G. L. Israel, A. Tiengo, R. Perna, R. Turolla, S. Zane, P. Esposito, G. A. Rodríguez Castillo, V. Graber, A. Possenti, C. Dehman, M. Ronchi, S. Loru
Format:	Artigo
Jezik:	Inglês
Izdano:	IOP Publishing 2023-01-01
Serija:	The Astrophysical Journal
Teme:	Neutron stars Magnetars
Online dostop:	https://doi.org/10.3847/1538-4357/aca528
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