Nova KT Eri 2009: Infrared studies of a very fast and small amplitude He/N nova

TL;DR

This study presents near-infrared spectroscopic and photometric observations of the fast, small-amplitude He/N nova KT Eri 2009, revealing its spectral features, light curve behavior, distance, and potential bipolar outflow, contributing to understanding nova classifications.

Contribution

First detailed infrared observational analysis of KT Eri, providing insights into its spectral features, rapid evolution, and possible recurrent nature, which enhances nova classification knowledge.

Findings

KT Eri is a very fast nova with t2 = 5.7 days.

Spectra show strong He I, H I, and O I emission lines.

Evidence suggests a bipolar outflow in the ejecta.

Abstract

We present near-infrared spectroscopic and photometric observations of the nova KT Eridani taken during the first 100 days following its discovery in 2009 November. The JHK spectra of the object have been taken from the Mount Abu Infrared Observatory using the Near-Infrared Imager/Spectrometer. The spectra, typical of the He/N class novae, show strong He I emission lines together with H I and O I emission features. The H I, Pa-beta and Br-gamma spectral lines and the He I line at 2.0581 micron show broad wings with a relatively narrow central component. The broad wings extend to 1900 km/s while the central component has FWHM of 2100 km/s. The V and near-infrared JHK light curves show an additional small amplitude outburst near 40 days after optical maximum. The distance to the nova d = 6.3 +/- 0.1 kpc is derived using the MMRD relation and the estimated value of t2 = 5.7 +/- 0.3 days. The small value of t2 places KT Eri in the class of very fast novae. Using the value of the distance to the nova d, we estimate the height of the nova to be z = 3.3 +/- 0.1 kpc below the galactic plane. We have also calculated the upper limit for the ejecta mass for KT Eri to be in the range 2.4-7.4 x 10^(-5) Msun. Kinematic evidence is presented from the shape of the line profiles for a possible bipolar flow. We analyze the temporal evolution of the continuum and also discuss the possibility of KT Eri being a recurrent nova.