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Georgakarakos, Nikolaos; Eggl, Siegfried
Monthly notices of the Royal Astronomical Society. Letters, 07/2019, Letnik: 487, Številka: 1Journal Article
ABSTRACT We investigate the hypothesis that the size of the habitable zone around hardened binaries in dense star-forming regions increases. Our results indicate that this hypothesis is essentially incorrect. Although certain binary star configurations permit extended habitable zones, such set-ups typically require all orbits in a system to be near-circular. In all other cases, planets can only remain habitable if they display an extraordinarily high climate inertia.
