pith:S356Y3FX
Early emission characterization of TDE 2025aarm
Early multi-wavelength data on TDE 2025aarm indicate its initial emission arises from circularization shocks under a delayed accretion picture.
arxiv:2603.20123 v3 · 2026-03-20 · astro-ph.HE
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Claims
Our analysis suggests that the early emission from TDE 2025aarm is powered by circularization shocks, and that the delayed accretion scenario best describes the observed features.
The optical light curves are well described by the fallback of a 0.16 solar mass star onto a 2x10^7 solar mass black hole, which assumes the standard TDE fallback model applies without significant systematic uncertainties or alternative emission mechanisms.
Early multi-wavelength data from TDE 2025aarm indicate emission powered by circularization shocks with delayed accretion onto a ~2x10^7 solar mass black hole.
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| First computed | 2026-06-24T01:15:02.045515Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/S356Y3FXXTMA3LI6NNKHGXJ75E \
| jq -c '.canonical_record' \
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Canonical record JSON
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