A circumbinary protoplanetary disc in a polar configuration

Abstract

Nearly all young stars are initially surrounded by `protoplanetary' discs of gas and dust, and in the case of single stars at least 30\% of these discs go on to form planets. The process of protoplanetary disc formation can result in initial misalignments, where the disc orbital plane is different to the stellar equator in single star systems, or to the binary orbital plane in systems with two stars. A quirk of the dynamics means that initially misaligned `circumbinary' discs -- those that surround two stars -- are predicted to evolve to one of two possible stable configurations, one where the disc and binary orbital planes are coplanar, and one where they are perpendicular (a `polar' configuration). Prior work has found coplanar circumbinary discs, but no polar examples were known until now. Here we report the first discovery of a protoplanetary circumbinary disc in the polar configuration, supporting the predictions that such discs should exist. The disc shows some characteristics that are similar to discs around single stars, and that are attributed to dust growth. Thus, the first stages of planet formation appear able to proceed in polar circumbinary discs.

Submitted version - do not read. Published in Nature Astronomy, free PDF at https://rdcu.be/bgNSO

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Cited by in corpus (4)

• A statistically significant lack of debris discs in medium separation binary systems
• Distinguishing Polar and Co-planar Circumbinary Exoplanets by Eclipsing Timing Variations
• The binary mass ratios of circumbinary planet hosts
• Birth environment of circumbinary planets: are there CBPs on the inclined orbits?