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astro-ph.HE2017★ 16 cited
The low luminosity behaviour of the 4U 0115+63 Be/X-ray transient
Alicia Rouco Escorial, Ann-Sofie Bak Nielsen, Rudy Wijnands +3
The Be/X-ray transient 4U 0115+63 exhibited a giant, type-II outburst in October 2015. The source did not decay to its quiescent state but settled in a meta-stable plateau state (a…
astro-ph.HE2017★ 12 cited
The X-ray Pulsar 2A 1822-371 as a Super Eddington source
A. Bak Nielsen, A. Patruno, C. D'Angelo
The low mass X-ray binary 2A 1822-371 is an eclipsing system with an accretion disc corona and with an orbital period of 5.57 hr. The primary is an 0.59 s X-ray pulsar with a propo…