X-Ray Observations of Nova Scorpii 2023 (V1716 Sco) in Outburst

Nova Scorpii 2023 (V1716 Sco) was first detected as a luminous supersoft X-ray source (SSS) 93 days after outburst and continued emitting soft X-rays for over 2 months, until it was too close to the Sun to observe. The nova was monitored with the Swift X-ray Telescope and the Neutron Star Interior C...

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Autors principals:	John T. Worley, Marina Orio, Andrej Dobrotka, Jozef Magdolen, Kim Page, Ehud Behar, Jeremy J. Drake, Sharon Mitrani
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Novae White dwarf stars Cataclysmic variable stars X-ray astronomy Time domain astronomy High energy astrophysics
Accés en línia:	https://doi.org/10.3847/1538-4357/ae157b
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