Selaus tekijän mukaan kokoelmassa Rinnakkaistallenteet
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High-energy characteristics of the accretion-powered millisecond pulsar IGR J17591-2342 during its 2018 outburst: XMM-Newton, NICER, NuSTAR, and INTEGRAL view of the 0.3-300 keV X-ray band
L. Kuiper; S.S. Tsygankov; M. Falanga; I.A. Mereminskiy; D.K. Galloway; J. Poutanen; Z. LiIGR J17591−2342 is an accreting millisecond X-ray pulsar, discovered with INTEGRAL, which went into outburst around July 21, 2018. To better understand the physics acting in these systems during the outburst episode, we ... -
The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars
A. Papitto; M. Falanga; W. Hermsen; S. Mereghetti; L. Kuiper; J. Poutanen; E. Bozzo; F. Ambrosino; F. Coti Zelati; V. De Falco; D. de Martino; T. Di Salvo; P. Esposito; C. Ferrigno; M. Forot; D. Götz; C. Gouiffes; R. Iaria; P. Laurent; J. Li; Z. Li; T. Mineo; P. Moran; A. Neronov; A. Paizis; N. Rea; A. Riggio; A. Sanna; V. Savchenko; A. Słowikowska; A. Shearer; A. Tiengo; D. F. Torres<p>In the last 25 years, a new generation of X-ray satellites imparted a significant leap forward in our knowledge of X-ray pulsars. The discovery of accreting and transitional millisecond pulsars proved that disk accretion ...