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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Үндсэн зохиолчид:	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
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	IOP Publishing 2023-01-01
Цуврал:	The Astrophysical Journal
Нөхцлүүд:	Neutron stars Magnetars
Онлайн хандалт:	https://doi.org/10.3847/1538-4357/aca528
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!