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Abstract

Context. Brown dwarfs are transition objects between stars and planets that are still poorly understood, for which several competing mechanisms have been proposed to describe their formation. Mass measurements are generally difficult to carry out for isolated objects as well as for brown dwarfs orbiting low-mass stars, which are often too faint for a spectroscopic follow-up.

Item Type: Article
Uncontrolled Keywords: gravitational lensing: micro / binaries: general / brown dwarfs / stars: low-mass
Subjects: Q Science > Q Science (General)
Q Science > QB Astronomy
Divisions: Faculty of Natural Sciences > School of Chemical and Physical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 08 Aug 2022 12:42
Last Modified: 08 Aug 2022 12:42
URI: https://eprints.keele.ac.uk/id/eprint/11244

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