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- W2949692080 abstract "Most young low-mass stars are born as binary systems, and circumstellar disks have recently been observed around the individual components of proto-binary systems (e.g. L1551-IRS5). Thus planets and planetary systems are likely to form around the individual stellar components in sufficiently wide binary systems. However, a good fraction of planets born in binary systems will in the long run be subject to ejection due to gravitational perturbations. Therefore, we expect that there should exist a free-floating population of Jupiter-like or even Earth-like planets in interstellar space. There is hope to detect the free-floating Jupiters through gravitational microlensing observations towards the Galactic Bulge, especially with large-format detectors in the near-infrared (e.g. with VISTA or NGST), on timescales of a few days." @default.
- W2949692080 created "2019-06-27" @default.
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- W2949692080 date "2001-07-18" @default.
- W2949692080 modified "2023-09-27" @default.
- W2949692080 title "A free-floating planet population in the Galaxy?" @default.
- W2949692080 hasPublicationYear "2001" @default.
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