A multiwavelength light curve analysis of the classical nova KT Eri: Optical contribution from a large irradiated accretion disk
Izumi Hachisu, Mariko Kato, Frederick M. Walter

TL;DR
This study models the optical and X-ray light curves of KT Eri, revealing a large irradiated accretion disk's role during outburst and estimating key system parameters, concluding KT Eri is likely not a recurrent nova.
Contribution
The paper presents a detailed light curve analysis of KT Eri, incorporating a large irradiated disk model, and derives system parameters, providing new insights into its classification and outburst behavior.
Findings
White dwarf mass estimated at 1.3 solar masses
Distance to KT Eri determined as 4.2 kpc
KT Eri is likely not a recurrent nova
Abstract
KT Eri is a classical nova which went into outburst in 2009. Recent photometric analysis in quiescence indicates a relatively longer orbital period of 2.6 days, so that KT Eri could host a very bright accretion disk during the outburst like in the recurrent nova U Sco, the orbital period of which is 1.23 days. We reproduced the optical light curve as well as the supersoft X-ray light curve of KT Eri in outburst, assuming a large irradiated disk during a nova wind phase of the outburst while a normal size disk after the nova winds stop. This result is consistent with the temporal variation of wide-band brightness that varies almost with the intermediate-band Str\"omgren brightness, because the flux is dominated by continuum radiation, the origin of which is a photospheric emission from the very bright disk. We obtained the white dwarf mass to be $M_{\rm WD}= 1.3\pm0.02…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · High-pressure geophysics and materials
