A Revised Historical Light Curve of Eta Carinae and the Timing of Close Periastron Encounters
Nathan Smith, David J. Frew

TL;DR
This paper revises the historical light curve of eta Carinae's 19th-century eruption, revealing brief eruptions resembling supernova impostors and analyzing their timing relative to the star's binary orbit.
Contribution
It uncovers and corrects historical brightness estimates, providing a revised light curve and analyzing the relationship between eruptions and periastron passages in eta Carinae.
Findings
Revised light curve shows two brief eruptions in 1838 and 1843.
The 1844 brightening was not associated with periastron.
The 1890 eruption's brightening began at periastron but was not directly triggered.
Abstract
The historical light curve of the 19th century "Great Eruption" of etaCar provides a striking record of violent instabilies encountered by the most massive stars. We report and analyze newly uncovered historical estimates of the visual brightness of etaCar during its eruption, and we correct some mistakes in the original record. The revised light curve looks substantially different from previous accounts: it shows two brief eruptions in 1838 and 1843 that resemble modern supernova impostors, while the final brightening in December 1844 marks the time when etaCar reached its peak brightness. We consider the timing of brightening events as they pertain to the putative binary system in etaCar: (1) The brief 1838 and 1843 events peaked within weeks of periastron if the pre-1845 orbital period is shorter than at present due to the mass loss of the eruption. Each event lasted only 100 days.…
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