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19992025
most citedThe formation of very wide binaries during the star cluster dissolution phase

195 citations · 546 across the 15 of their papers we have counts for

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5 papers · 1 filter

astro-ph.SR2025

Can planet-planet binaries survive in star-forming regions?

Richard J. Parker, Simon P. Goodwin, Jessica L. Diamond

Significant numbers of free-floating planetary-mass objects have been discovered in nearby star-forming regions by the James Webb Space Telescope, including a substantial number (4…

astro-ph.SR2015★ 24 cited

The dynamical evolution of low-mass hydrogen-burning stars, brown dwarfs and planetary-mass objects formed through disc fragmentation

Yun Li, M. B. N. Kouwenhoven, D. Stamatellos +1

Theory and simulations suggest that it is possible to form low-mass hydrogen-burning stars, brown dwarfs and planetary-mass objects via disc fragmentation. As disc fragmentation re…

astro-ph.SR2014★ 15 cited

How does a low-mass cut-off in the stellar IMF affect the evolution of young star clusters?

M. B. N. Kouwenhoven, S. P. Goodwin, R. de Grijs +2

We investigate how different stellar initial mass functions (IMFs) can affect the mass loss and survival of star clusters. We find that IMFs with radically different low-mass cut-o…

astro-ph.SR2011★ 57 cited

Disc Frequencies for Brown Dwarfs in the Upper Scorpius OB Association: Implications for Brown Dwarf Formation Theories

B. Riaz, N. Lodieu, S. Goodwin +2

We have investigated the brown dwarf (BD) and stellar disc fractions in the Upper Scorpius OB Association (USco) and compared them with several other young regions. We have compile…

astro-ph.SR2011★ 1 cited

The origin of very wide binary stars

M. B. N. Kouwenhoven, S. P. Goodwin, Melvyn B. Davies +3

A large population of fragile, wide (> 1000 AU) binary systems exists in the Galactic field and halo. These wide binary stars cannot be primordial because of the high stellar densi…