Discovery of a New Flaring Class in GRS 1915+105 Using AstroSat

The highly variable black hole X-ray binary GRS 1915+105 has shown many flaring classes when the source oscillates between the high soft state (HS) and the hard intermediate state with a transition time of less than 10 s. The X-ray flux is anticorrelated with the hardness ratio (HR2) during these X-...

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Bibliographic Details
Main Authors: Ruchika Dhaka, J. S. Yadav, Ranjeev Misra, Pankaj Jain
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adc381
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