What type of study is this?

This is a Quantitative Study study.

October 20, 2025Open Access

Can GRB 250702B be explained as the tidal disruption of a white dwarf by an intermediate mass black hole? Yes

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Authors

RERob AJ Eyles-FerrisUniversity of Leicester AKAndrew P. KingKing's College London RSR. L. C. StarlingUniversity of Leicester

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Implication

Analysis reveals gamma-ray emissions linked to a white dwarf interacting with an intermediate mass black hole, suggesting new insights into high energy transients.

Key Points

The findings indicate that the features of GRB 250702B align with a model of a white dwarf interacting with a black hole.
Gamma-ray emissions can be explained by shocks from debris streams colliding at the orbital period of the star.
Accretion on the black hole generates X-rays but does not fully account for the gamma-ray emission observed.
Future studies on jet properties will help refine the proposed model and its implications for understanding high energy transients.

Cite This Study

Eyles-Ferris et al. (2025) studied this question.

synapsesocial.com/papers/68f6196ee0bbbc94fac3642e https://doi.org/10.48550/arxiv.2509.22843

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Implication

Analysis reveals gamma-ray emissions linked to a white dwarf interacting with an intermediate mass black hole, suggesting new insights into high energy transients.

Can GRB 250702B be explained as the tidal disruption of a white dwarf by an intermediate mass black hole? Yes

Discussion

Member takes

Implication

Key Points

Cite This Study

Can GRB 250702B be explained as the tidal disruption of a white dwarf by an intermediate mass black hole? Yes

Discussion

Member takes

Implication

Key Points

Cite This Study

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