The Nova KT Eri Is a Recurrent Nova With a Recurrence Time-Scale of 40-50 Years
Bradley E. Schaefer, Frederick M. Walter, Rebekah Hounsell, Yael, Hillman

TL;DR
This study confirms KT Eri as a recurrent nova with a recurrence time-scale of 40-50 years, based on extensive photometric, spectroscopic, and archival data analysis, revealing its high white dwarf mass and accretion rate.
Contribution
The paper provides the first detailed analysis establishing KT Eri as a recurrent nova with a well-constrained recurrence interval of 40-50 years, combining multi-wavelength observations and archival data.
Findings
KT Eri has an orbital period of 2.61595 days.
The companion star's temperature is approximately 6200 K.
The white dwarf mass is about 1.25 solar masses.
Abstract
KT Eridani was a very fast nova in 2009 peaking at V=5.42 mag. We marshal large data sets of photometry to finally work out the nature of KT Eri. From the TESS light curve, as confirmed with our radial velocity curve, we find an orbital period of 2.61595 days. With our 272 spectral energy distributions from simultaneous BVRIJHK measures, the companion star has a temperature of 6200500 K. Our century-long average in quiescence has V=14.5. With the Gaia distance (5110 parsecs), the absolute magnitude is +0.70.3. We converted this absolute magnitude (corrected to the disc light alone) to accretion rates, with a full integration of the alpha-disc model. This accretion rate is very high at 3.5x10 solar masses per year. Our search and analysis of archival photographs shows that no eruption occurred from 1928--1954 or after 1969. With our analysis of the…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astronomical Observations and Instrumentation · Gamma-ray bursts and supernovae
