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A model on transition between steady states of sub-Keplerian accretion discs: implication for spectral states and hot corona above the disc

Published Online: 2024-05-27

Published Print: 2024-05

Authors

Ajay, Arunima

Rajesh, S. R.

Singh, Nishant K.
Funding

Funding for this research was provided by:

CSIR-UGC Fellowship, India
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Text and Data Mining valid from 2024-05-01

Version of Record valid from 2024-05-01
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Article History

Received: 28 November 2023

Accepted: 15 May 2024

First Online: 27 May 2024

Declarations

:

: The authors declare no competing interests.

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