Was there a (super)nova in 1408?
Boshun Yang, Nikolaus Vogt, Susanne M Hoffmann

TL;DR
This study re-evaluates the 1408 CE Chinese historical record of a luminous transient, suggesting it was likely a nova or supernova, and explores possible modern counterparts like CK Vul, integrating historical texts with astrophysical data.
Contribution
It combines detailed historical analysis with modern astrophysical data to identify the 1408 event as a probable nova or supernova, providing new insights into ancient stellar phenomena.
Findings
The 1408 event was stationary, luminous, and consistent with a slow nova or supernova.
CK Vul is a plausible modern remnant related to the 1408 transient.
Historical records can be effectively integrated with modern data to study ancient astronomical events.
Abstract
The 1408 CE "guest star" recorded in Chinese historical texts presents a compelling case for identifying a historical stellar transient. While previous studies debated its nature as a meteor, comet, or nova, we re-evaluate the event using original Ming Dynasty records, including a newly found memorial from the imperial court. The object, described as stationary for over ten days, yellow, and luminous (resembling a "Zhou Bo virtue star"), is inconsistent with cometary behavior. Positional analysis locates it near the Niandao asterism (modern Cygnus-Vulpecula region) within the Milky Way, with a derived brightness of -4 to 0 mag. Light-curve stability over ten days and color descriptions align with a slow nova or a supernova. We cross-correlated the historical coordinates with modern catalogs and found a few possible counterparts. Among them, CK Vul - a luminous red nova remnant from 1670…
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