The HOSTS Survey: Suspected variable dust emission and constraints on companions around {\theta} Boo

TL;DR

This study investigates suspected variable exozodiacal dust around { heta} Boo, using multi-epoch nulling and high-contrast imaging to model dust distribution, constrain potential companions, and explore dust variability near the habitable zone.

Contribution

It provides new multi-epoch nulling observations and dust modeling of { heta} Boo, offering constraints on dust grain size, distribution, and potential companions, and discusses dust variability over time.

Findings

Detected excess dust emission near the habitable zone.

Constrained dust grain size to approximately 3-5 micrometers.

Tentative evidence of increased dust brightness between 2017 and 2023.

Abstract

During the HOSTS survey by the LBTI, an excess emission from the main sequence star {\theta} Boo (F7V spectral type, 14.5pc distance) was observed. This excess indicates the presence of exozodiacal dust near the habitable zone (HZ) of the star. Previous observations from Spitzer and Herschel showed no sign of outer cold dust within their respective detection limits. Additional nulling and high-contrast AO observations were taken to spatially constrain the dust distribution, search for variability, and directly image potential companions in the system. This study presents the results of these observations and provides an interpretation of the inner system's architecture. The star was observed using the LBTI's N'-band nulling mode during three epochs in 2017, 2018, and 2023. The dust distribution is modeled and constrained for each epoch using the standard LBTI nulling pipeline, assuming a vertically thin disk with a face-on inclination. In addition, high-contrast AO observations are performed in the L'-band and H-band to constrain the presence of substellar companions around the star. Several solutions are found for the dust distribution, and for each epoch. However, the LBTI nulling observations are not able to discriminate between them. Using the upper limits from previous observations, we constrain the representative size of the dust grains around 3-5$\mu$m. A tentative increase in dust brightness is also measured at the Earth-equivalent insolation distance between 2017 and 2023. Several options are considered to explain the origin of the observed dust and its variability, but no clear sources could be identified from the current observations. Partly because our high-contrast AO observations could only constrain the presence of companions down to $11M_\text{Jup}$ at 1.3" separation.