Infrared spectroscopy of the merger candidate KIC 9832227

TL;DR

This study presents infrared spectroscopic data of the contact binary star KIC 9832227, aiming to characterize its components and environment to better understand its predicted merger event in 2022.

Contribution

It provides the first near-infrared spectrum analysis of KIC 9832227, revealing stellar parameters and chromospheric activity relevant to its merger process.

Findings

Infrared spectrum best fitted by a single star with T_eff=5920K

Presence of chromosphere indicated by CaII triplet and H lines

HeI absorption suggests circumstellar activity

Abstract

Context: It has been predicted that the object KIC 9832227 - a contact binary star - will undergo a merger in 2022.2+/-0.7. We describe the near infrared spectrum of this object as an impetus to obtain pre-merger data. Aims: We aim to characterise (i)~the nature of the individual components of the binary and (ii)~the likely circumbinary environment, so that the merger - if and when it occurs - can be interpreted in an informed manner. Methods: We use infrared spectroscopy in the wavelength range 0.7micron - 2.5microns, to which we fit model atmospheres to represent the individual stars. We use the binary ephemeris to determine the orbital phase at the time of observation. Results: We find that the infrared spectrum is best fitted by a single component having effective temperature 5920K, log[g]=4.1 and solar metallicity, consistent with the fact that the system was observed at conjunction. Conclusions: The strength of the infrared H lines is consistent with a high value of log[g], and the strength of the CaII triplet indicates the presence of a chromosphere, as might be expected from rapid stellar rotation. The HeI absorption we observe likely arises in He excited by coronal activity in a circumstellar envelope, suggesting that the weakness of the CaII triplet is also likely chromospheric in origin.