Light echoes reveal an unexpectedly cool Eta Carinae during its 19th-century Great Eruption
A. Rest, J. L. Prieto, N. R. Walborn, N. Smith, F. B. Bianco, R., Chornock, D. L. Welch, D. A. Howell, M. E. Huber, R. J. Foley, W. Fong, B., Sinnott, H. E. Bond, R. C. Smith, I. Toledo, D. Minniti, K. Mandel

TL;DR
Light echoes from Eta Carinae's 19th-century eruption reveal it was unexpectedly cool, challenging existing models and suggesting alternative physical mechanisms like blast waves influenced the event.
Contribution
This study provides the first spectral analysis of light echoes from Eta Carinae's Great Eruption, revealing a cooler outburst temperature than predicted by standard models.
Findings
Spectra show only blueshifted absorption lines consistent with expansion speeds.
Effective temperature of the eruption was ~5000 K, cooler than standard models predict.
Results suggest alternative mechanisms like blast waves influenced the eruption.
Abstract
Eta Carinae (Eta Car) is one of the most massive binary stars in the Milky Way. It became the second-brightest star in the sky during its mid-19th century "Great Eruption," but then faded from view (with only naked-eye estimates of brightness). Its eruption is unique among known astronomical transients in that it exceeded the Eddington luminosity limit for 10 years. Because it is only 2.3 kpc away, spatially resolved studies of the nebula have constrained the ejected mass and velocity, indicating that in its 19th century eruption, Eta Car ejected more than 10 M_solar in an event that had 10% of the energy of a typical core-collapse supernova without destroying the star. Here we report the discovery of light echoes of Eta Carinae which appear to be from the 1838-1858 Great Eruption. Spectra of these light echoes show only absorption lines, which are blueshifted by -210 km/s, in good…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
