The SN 1987A Link to Others and Gamma-Ray Bursts
John Middleditch

TL;DR
This paper proposes that SN 1987A originated from a double degenerate merger, linking it to gamma-ray bursts and millisecond pulsars, challenging existing models and suggesting a unified explanation for various astrophysical phenomena.
Contribution
It introduces a new interpretation of SN 1987A as a double degenerate merger, connecting it to gamma-ray bursts and millisecond pulsars, and questions the necessity of exotic models.
Findings
SN 1987A's features support a double degenerate merger origin.
Long-soft GRBs can result from jet impacts in such mergers.
Millisecond pulsars and some supernovae are consistent with DD merger origins.
Abstract
Early measurements of SN 1987A can be interpreted in light of a beam/jet (BJ), with a collimation factor >10,000, which impacted polar ejecta (PE) to produce the "Mystery Spot" (MS), ~24 lt-d away. Other details of SN 1987A suggest that it came from a merger of 2 stellar cores of a common envelope (CE) binary, i.e. a "double degenerate" (DD) SN. Even having to penetrate the CE, the BJ may have caused a long-soft (l)GRB upon hitting the PE, thus DD can produce lGRBs. Because DD must be the dominant merger/SN mechanism in elliptical galaxies (EGs), where only short, hard GRBs (sGRBs) have been observed, DD without CE or PE must also produce sGRBs, and thus NS-NS mergers may not make GRBs as we know them, and/or be as common as previously thought. Millisecond pulsars (MSPs) in the non-core-collapsed globular clusters are also 99% DD-formed from WD-WD merger, consistent with their 2.10 ms…
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Taxonomy
TopicsGamma-ray bursts and supernovae
