Novae, supernovae, or something else? -- (Super-)nova highlights from Hoffmann & Vogt are quite certainly comets (AD 668 and 891)
Ralph Neuhaeuser (AIU Jena), Dagmar L. Neuhaeuser, Jesse Chapman (NY, University)

TL;DR
This paper critically examines Hoffmann & Vogt's historical transient catalog, arguing that their identifications of certain Chinese records as supernovae are likely misinterpretations, and emphasizing the importance of proper historical and astronomical context.
Contribution
The paper provides a detailed critique of Hoffmann & Vogt's candidate identifications, highlighting translation, dating, and interpretative errors, and clarifies that the records are more consistent with comet sightings.
Findings
The AD 668 and 891 records are strongly supported as comet sightings.
The AD 667 record is a misdated doublet of 668.
Hoffmann & Vogt's candidate list lacks solid foundation and should be used cautiously.
Abstract
Galactic novae and supernovae can be studied by utilizing historical observations, yielding explosion time, location on sky~etc. Recent publications by Hoffmann & Vogt present CVs, supernova remnants, planetary nebulae etc. as potential counterparts based on their list of historically reported transients from the Classical Chinese text corpus. Since their candidate selection neglects the state-of-the-art (e.g. Stephenson \& Green), and since it includes `broom stars' and `fuzzy stars', i.e. probable comets, we investigate their catalogue in more detail. We discuss here their two highlights, the suggestion of two `broom star' records dated AD 667 and 668 as one historical supernova and of the `guest star' of AD 891 as recurrent nova U Sco. The proposed positional search areas are not justified due to translation and dating problems, source omission, as well as misunderstandings of…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Australian Indigenous Culture and History · Historical Astronomy and Related Studies
