An X-ray Shell Reveals the Supernova Explosion for Galactic Microquasar SS 433
Yi-Heng Chi, Jiahui Huang, Ping Zhou, Hua Feng, Xiang-Dong Li, Sera B., Markoff, Samar Safi-Harb, Laura Olivera-Nieto

TL;DR
This study reports the discovery of an X-ray shell near the microquasar SS 433, providing evidence that some black holes originate from supernova explosions, with implications for understanding black hole formation and cosmic ray acceleration.
Contribution
The paper presents observational evidence linking a supernova remnant to the formation of a stellar-mass black hole in SS 433, supporting the canonical supernova explosion model.
Findings
An X-ray shell associated with SS 433 indicates a supernova origin.
The shell's spectrum suggests it was created 20-30 kyr ago by a supernova.
The progenitor star was likely more massive than 25 solar masses.
Abstract
How black holes are formed remains an open and fundamental question in Astrophysics. Despite theoretical predictions, it lacks observations to understand whether the black hole formation experiences a supernova explosion. Here we report the discovery of an X-ray shell north of the Galactic micro-quasar SS 433 harboring a stellar-mass black hole spatially associated with radio continuum and polarization emissions, and an HI cloud. Its spectrum can be reproduced by a 1-keV under-ionized plasma, from which the shell is inferred to have been created by a supernova explosion 20-30 kyr ago and its properties constitute evidence for canonical SN explosions to create some black holes. Our analysis precludes other possible origins including heated by jets or blown by disk winds. According to the lower mass limit of the compact object in SS 433, we roughly deduced that the progenitor should be…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
