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Resolved Kinematics of Runaway and Field OB Stars in the Small Magellanic Cloud
M. S. Oey, J. Dorigo Jones, N. Castro +6
We use GAIA DR2 proper motions of the RIOTS4 field OB stars in the Small Magellanic Cloud (SMC) to study the kinematics of runaway stars. The data reveal that the SMC Wing has a sy…
The Close Binary Fraction of Solar-type Stars is Strongly Anti-correlated with Metallicity
Maxwell Moe, Kaitlin M. Kratter, Carles Badenes
There is now strong evidence that the close binary fraction (P < 10 days; a < 10 AU) of solar-type stars ( = 0.6-1.5M) decreases significantly with metallicity.…
Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
J. Klencki, M. Moe, W. Gladysz +3
The distributions of the initial main-sequence binary parameters are one of the key ingredients in obtaining evolutionary predictions for compact binary (BH-BH / BH-NS / NS-NS) mer…
Young and eccentric: the quadruple system HD 86588
Andrei Tokovinin, Hank Corbett, Octavi Fors +4
High-resolution spectroscopy and speckle interferometry reveal the young star HD 86588 as a quadruple system with a 3-tier hierarchy. The 0.3" resolved binary A,B with an estimated…