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Table · dataset · 2024

The lowest mass ratio contact binary

Listed in IVOA Registry (Virtual Observatory)

This paper presents the first analysis of the contact binary TYC 3801-1529-1.

Description

We observed four sets of multiple bands complete light curves and one set of radial velocity curve of the primary component. Based on a simultaneous investigation of our observed and TESS light curves and the radial velocity curve, we found that TYC 3801-1529-1 is an extremely low-mass-ratio, medium contact binary with q=0.0356, with the contribution of the third light at a level of about 10%.

Its mass ratio is lower than V1187 Her, making TYC 3801-1529-1 the lowest mass-ratio contact binary ever found in the universe. The light curves observed in 2022 are asymmetric, which is aptly explained by a hot spot on the primary component. A 16-year eclipse timings analysis indicates a secular increase orbital period with a rate of dp/dt=7.96(+/-0.35)*10^-7^d/yr.

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We studied the stability of this target and identified that not only the value of J_spin_/J_orb_, but also the mass ratio surpass the unstable boundary. Hence, TYC 3801-1529-1 presents a challenge to theoretical research and ought to be considered a progenitor of a contact binary merger.

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Catalogue records · 2

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Astronomical sciences 71%
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