On dust evolution in planet-forming discs in binary systems – II. Comparison with Taurus and ρ Ophiuchus (sub-)millimetre observations: discs in binaries have small dust sizes
ABSTRACT The recently discovered exoplanets in binary or higher order multiple stellar systems sparked a new interest in the study of protoplanetary discs in stellar aggregations. Here, we focus on disc solids, as they make up the reservoir out of which exoplanets are assembled and dominate (sub-)mi...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2021-10, Vol.507 (2), p.2531-2549 |
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Format: | Artikel |
Sprache: | eng |
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