Discovery of a New Phase-transient Cyclotron Line in A0535+26: Constraints on the Accretion Geometry

Discovery of a New Phase-transient Cyclotron Line in A0535+26: Constraints on the Accretion Geometry

In 2020 November, A0535+26 underwent one of its brightest outbursts, reaching nearly 12 Crab in X-ray flux. Observed by Insight-HXMT, NuSTAR, NICER, and AstroSat, this event provided valuable insights into Be/X-ray binaries. The pulse profiles evolved significantly with luminosity, transitioning fro...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy: Ashwin Devaraj, Biswajit Paul, Varun Bhalerao, Dipanjan Mukherjee
Format: Artykuł
Język:English
Wydane: IOP Publishing 2025-01-01
Seria:The Astrophysical Journal
Hasła przedmiotowe:
X-ray binary stars
High mass x-ray binary stars
X-ray astronomy
Binary pulsars
Neutron stars
Dostęp online:https://doi.org/10.3847/1538-4357/adb0c2

Internet

https://doi.org/10.3847/1538-4357/adb0c2

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