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The RS Oph Outburst of 2021 Monitored in X-Rays with NICER

The 2021 outburst of the symbiotic recurrent nova RS Oph was monitored with the Neutron Star Interior Composition Explorer Mission (NICER) in the 0.2–12 keV range from day one after the optical maximum, until day 88, producing an unprecedented, detailed view of the outburst development. The X-ray fl...

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Автори: Marina Orio, Keith Gendreau, Morgan Giese, Gerardo Juan M. Luna, Jozef Magdolen, Tod E. Strohmayer, Andy E. Zhang, Diego Altamirano, Andrej Dobrotka, Teruaki Enoto, Elizabeth C. Ferrara, Richard Ignace, Sebastian Heinz, Craig Markwardt, Joy S. Nichols, Michael L. Parker, Dheeraj R. Pasham, Songpeng Pei, Pragati Pradhan, Ron Remillard, James F. Steiner, Francesco Tombesi
Формат: Artigo
Мова:Inglês
Опубліковано: IOP Publishing 2023-01-01
Серія:The Astrophysical Journal
Предмети:
Novae
Recurrent novae
High energy astrophysics
X-ray transient sources
X-ray binary stars
Transient sources
Онлайн доступ:https://doi.org/10.3847/1538-4357/ace9bd
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